Astrophysics with the Laser Interferometer Space Antenna

Antoni A, MacLeod M, Ramirez-Ruiz E (2019) The Evolution of Binaries in a Gaseous Medium: Three-dimensional Simulations of Binary Bondi-Hoyle-Lyttleton Accretion. ApJ 884(1):22. https://doi.org/10.3847/1538-4357/ab3466 . arXiv:1901.07572 [astro-ph.HE]

Original

1901

Earlier work this paper cites.

Davé R, Anglés-Alcázar D, Narayanan D, Li Q, Rafieferantsoa MH, Appleby S (2019) SIMBA: Cosmological simulations with black hole growth and feedback. MNRAS 486(2):2827–2849. https://doi.org/10.1093/mnras/stz937 . arXiv:1901.10203 [astro-ph.GA]

Original

1901

Earlier work this paper cites.

Di Carlo UN, Giacobbo N, Mapelli M, Pasquato M, Spera M, Wang L, Haardt F (2019) Merging black holes in young star clusters. MNRAS 487(2):2947–2960. https://doi.org/10.1093/mnras/stz1453 . arXiv:1901.00863 [astro-ph.HE]

Original

1901

Earlier work this paper cites.

Kimpson T, Wu K, Zane S (2019b) Spatial dispersion of light rays propagating through a plasma in Kerr space-time. MNRAS 484(2):2411–2419. https://doi.org/10.1093/mnras/stz138 . arXiv:1901.03733 [astro-ph.HE]

Original

1901

Earlier work this paper cites.

Liptai D, Price DJ (2019) General relativistic smoothed particle hydrodynamics. MNRAS 485(1):819–842. https://doi.org/10.1093/mnras/stz111 . arXiv:1901.08064 [astro-ph.IM]

Original

1901

Earlier work this paper cites.

Marassi S, Graziani L, Ginolfi M, Schneider R, Mapelli M, Spera M, Alparone M (2019) Evolution of dwarf galaxies hosting GW150914-like events. MNRAS 484(3):3219–3232. https://doi.org/10.1093/mnras/stz170 . arXiv:1901.04494 [astro-ph.GA]

Original

1901

Earlier work this paper cites.

McNeill LO, Mardling RA, Müller B (2020) Gravitational waves from dynamical tides in white-dwarf binaries. MNRAS 491(2):3000–3012. https://doi.org/10.1093/mnras/stz3215 . arXiv:1901.09045 [astro-ph.HE]

Original

1901

Earlier work this paper cites.

Nevin R, Blecha L, Comerford J, Greene J (2019) Accurate Identification of Galaxy Mergers with Imaging. ApJ 872(1):76. https://doi.org/10.3847/1538-4357/aafd34 . arXiv:1901.01975 [astro-ph.GA]

Original

1901

Earlier work this paper cites.

van den Heuvel EPJ (2019) High-Mass X-ray Binaries: progenitors of double compact objects. In: Oskinova LM, Bozzo E, Bulik T, Gies DR (eds) IAU Symposium. IAU Symposium, vol 346. pp 1–13. https://doi.org/10.1017/S1743921319001315 . arXiv:1901.06939 [astro-ph.HE]

Original

1901

Earlier work this paper cites.

van Son LAC, Barber C, Bahé YM, Schaye J, Barnes DJ, Crain RA, Kay ST, Theuns T, Dalla Vecchia C (2019) Galaxies with monstrous black holes in galaxy cluster environments. MNRAS 485(1):396–407. https://doi.org/10.1093/mnras/stz399 . arXiv:1901.03156 [astro-ph.GA]

Original

1901

Earlier work this paper cites.

Wise JH, Regan JA, O’Shea BW, Norman ML, Downes TP, Xu H (2019) Formation of massive black holes in rapidly growing pre-galactic gas clouds. Nature 566(7742):85–88. https://doi.org/10.1038/s41586-019-0873-4 . arXiv:1901.07563 [astro-ph.GA]

Original

1901

Earlier work this paper cites.

Banerjee S, Belczynski K, Fryer CL, Berczik P, Hurley JR, Spurzem R, Wang L (2020) BSE versus StarTrack: Implementations of new wind, remnant-formation, and natal-kick schemes in NBODY7 and their astrophysical consequences. A&A 639:A41. https://doi.org/10.1051/0004-6361/201935332 . arXiv:1902.07718 [astro-ph.SR]

Original

1902

Earlier work this paper cites.

Bellm EC, Kulkarni SR, Graham MJ, Dekany R, Smith RM, Riddle R, Masci FJ, et al (2019) The Zwicky Transient Facility: System Overview, Performance, and First Results. PASP 131(995):018002. https://doi.org/10.1088/1538-3873/aaecbe . arXiv:1902.01932 [astro-ph.IM]

Original

1902

Earlier work this paper cites.

Bortolas E, Mapelli M (2019) Can supernova kicks trigger EMRIs in the Galactic Centre? MNRAS 485(2):2125–2138. https://doi.org/10.1093/mnras/stz440 . arXiv:1902.04581 [astro-ph.GA]

Original

1902

Earlier work this paper cites.

Bustamante S, Springel V (2019) Spin evolution and feedback of supermassive black holes in cosmological simulations. MNRAS 490(3):4133–4153. https://doi.org/10.1093/mnras/stz2836 . arXiv:1902.04651 [astro-ph.GA]

Original

1902

Earlier work this paper cites.

Farrow N, Zhu XJ, Thrane E (2019) The Mass Distribution of Galactic Double Neutron Stars. ApJ 876(1):18. https://doi.org/10.3847/1538-4357/ab12e3 . arXiv:1902.03300 [astro-ph.HE]

Original

1902

Earlier work this paper cites.

Garavito-Camargo N, Besla G, Laporte CFP, Johnston KV, Gómez FA, Watkins LL (2019) Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud. ApJ 884(1):51. https://doi.org/10.3847/1538-4357/ab32eb . arXiv:1902.05089 [astro-ph.GA]

Original

1902

Earlier work this paper cites.

Gerosa D, Ma S, Wong KWK, Berti E, O’Shaughnessy R, Chen Y, Belczynski K (2019) Multiband gravitational-wave event rates and stellar physics. Phys. Rev. D 99(10):103004. https://doi.org/10.1103/PhysRevD.99.103004 . arXiv:1902.00021 [astro-ph.HE]

Original

1902

Earlier work this paper cites.

Hamilton C, Rafikov RR (2019b) Secular dynamics of binaries in stellar clusters - I. General formulation and dependence on cluster potential. MNRAS 488(4):5489–5511. https://doi.org/10.1093/mnras/stz1730 . arXiv:1902.01344 [astro-ph.GA]

Original

1902

Earlier work this paper cites.

Li KJ, Wu K, Singh D (2019) Spin dynamics of a millisecond pulsar orbiting closely around a massive black hole. MNRAS 485(1):1053–1066. https://doi.org/10.1093/mnras/stz389 . arXiv:1902.03146 [astro-ph.HE]

Original

1902

Earlier work this paper cites.

Masci FJ, Laher RR, Rusholme B, Shupe DL, Groom S, Surace J, Jackson E, Monkewitz S, Beck R, Flynn D, et al. (2019) The Zwicky Transient Facility: Data Processing, Products, and Archive. PASP 131(995):018003. https://doi.org/10.1088/1538-3873/aae8ac . arXiv:1902.01872 [astro-ph.IM]

Original

1902

Earlier work this paper cites.

Pearson WJ, Wang L, Trayford JW, Petrillo CE, van der Tak FFS (2019) Identifying galaxy mergers in observations and simulations with deep learning. A&A 626:A49. https://doi.org/10.1051/0004-6361/201935355 . arXiv:1902.10626 [astro-ph.GA]

Original

1902

Earlier work this paper cites.

Pfister H, Volonteri M, Dubois Y, Dotti M, Colpi M (2019b) The erratic dynamical life of black hole seeds in high-redshift galaxies. MNRAS 486(1):101–111. https://doi.org/10.1093/mnras/stz822 . arXiv:1902.01297 [astro-ph.GA]

Original

1902

Earlier work this paper cites.

Pillepich A, Nelson D, Springel V, Pakmor R, Torrey P, Weinberger R, Vogelsberger M, Marinacci F, Genel S, van der Wel A, et al. (2019) First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time. MNRAS 490(3):3196–3233. https://doi.org/10.1093/mnras/stz2338 . arXiv:1902.05553 [astro-ph.GA]

Original

1902

Earlier work this paper cites.

Randall L, Xianyu ZZ (2019b) Observing Eccentricity Oscillations of Binary Black Holes in LISA. arXiv e-prints arXiv:1902.08604. arXiv:1902.08604 [astro-ph.HE]

Original

1902

Earlier work this paper cites.

Shiber S, Iaconi R, De Marco O, Soker N (2019) Companion-launched jets and their effect on the dynamics of common envelope interaction simulations. MNRAS 488(4):5615–5632. https://doi.org/10.1093/mnras/stz2013 . arXiv:1902.03931 [astro-ph.SR]

Original

1902

Earlier work this paper cites.

Wevers T, Stone NC, van Velzen S, Jonker PG, Hung T, Auchettl K, Gezari S, Onori F, Mata Sánchez D, Kostrzewa-Rutkowska Z, et al. (2019) Black hole masses of tidal disruption event host galaxies II. MNRAS 487(3):4136–4152. https://doi.org/10.1093/mnras/stz1602 . arXiv:1902.04077 [astro-ph.HE]

Original

1902

Earlier work this paper cites.

Wong KWK, Baibhav V, Berti E (2019a) Binary radial velocity measurements with space-based gravitational-wave detectors. MNRAS 488(4):5665–5670. https://doi.org/10.1093/mnras/stz2077 . arXiv:1902.01402 [astro-ph.HE]

Original

1902

Earlier work this paper cites.

Almeida LA, de Almeida L, Damineli A, Rodrigues CV, Castro M, Ferreira Lopes CE, Jablonski F, do Nascimento J J D, Pereira MG (2019) Orbital Period Variation of KIC 10544976: Applegate Mechanism versus Light Travel Time Effect. AJ 157(4):150. https://doi.org/10.3847/1538-3881/ab0963 . arXiv:1903.09637 [astro-ph.SR]

Original

1903

Earlier work this paper cites.

Amaro-Seoane P (2019) Extremely large mass-ratio inspirals. Phys. Rev. D 99(12):123025. https://doi.org/10.1103/PhysRevD.99.123025 . arXiv:1903.10871 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Artale MC, Mapelli M, Giacobbo N, Sabha NB, Spera M, Santoliquido F, Bressan A (2019) Host galaxies of merging compact objects: mass, star formation rate, metallicity, and colours. MNRAS 487(2):1675–1688. https://doi.org/10.1093/mnras/stz1382 . arXiv:1903.00083 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Bassini L, Rasia E, Borgani S, Ragone-Figueroa C, Biffi V, Dolag K, Gaspari M, Granato GL, Murante G, Taffoni G, et al. (2019) Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations. A&A 630:A144. https://doi.org/10.1051/0004-6361/201935383 . arXiv:1903.03142 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Berry C, Hughes S, Sopuerta C, Chua A, Heffernan A, Holley-Bockelmann K, Mihaylov D, Miller C, Sesana A (2019) The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy. BAAS 51(3):42. arXiv:1903.03686 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Biava N, Colpi M, Capelo PR, Bonetti M, Volonteri M, Tamfal T, Mayer L, Sesana A (2019) The lifetime of binary black holes in Sérsic galaxy models. MNRAS 487(4):4985–4994. https://doi.org/10.1093/mnras/stz1614 . arXiv:1903.05682 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Corrales L, Mills BS, Heinz S, Williger GM (2019) The X-Ray Variable Sky as Seen by MAXI: The Future of Dust-echo Tomography with Bright Galactic X-Ray Bursts. ApJ 874(2):155. https://doi.org/10.3847/1538-4357/ab0c9b . arXiv:1903.08299 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Cutler C, Berti E, Holley-Bockelmann K, Jani K, Kovetz ED, Larson SL, Littenberg T, McWilliams ST, Mueller G, Randall L, et al. (2019) What can we learn from multi-band observations of black hole binaries? BAAS 51(3):109. arXiv:1903.04069 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Fan X, Barth A, Banados E, De Rosa G, Decarli R, Eilers AC, Farina EP, Greene J, Habouzit M, Jiang L, et al. (2019) The First Luminous Quasars and Their Host Galaxies. BAAS 51(3):121. arXiv:1903.04078 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Fragione G, Kocsis B (2019) Black hole mergers from quadruples. MNRAS 486(4):4781–4789. https://doi.org/10.1093/mnras/stz1175 . arXiv:1903.03112 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Fragione G, Loeb A (2019) Black hole-neutron star mergers from triples. MNRAS 486(3):4443–4450. https://doi.org/10.1093/mnras/stz1131 . arXiv:1903.10511 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Ginat YB, Glanz H, Perets HB, Grishin E, Desjacques V (2020) Gravitational waves from in-spirals of compact objects in binary common-envelope evolution. MNRAS 493(4):4861–4867. https://doi.org/10.1093/mnras/staa465 . arXiv:1903.11072 [astro-ph.SR]

Original

1903

Earlier work this paper cites.

Gourgoulhon E, Le Tiec A, Vincent FH, Warburton N (2019) Gravitational waves from bodies orbiting the Galactic center black hole and their detectability by LISA. A&A 627:A92. https://doi.org/10.1051/0004-6361/201935406 . arXiv:1903.02049 [gr-qc]

Original

1903

Earlier work this paper cites.

Hoang BM, Naoz S, Kocsis B, Farr WM, McIver J (2019) Detecting Supermassive Black Hole-induced Binary Eccentricity Oscillations with LISA. ApJ 875(2):L31. https://doi.org/10.3847/2041-8213/ab14f7 . arXiv:1903.00134 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Kelley L, Charisi M, Burke-Spolaor S, Simon J, Blecha L, Bogdanovic T, Colpi M, Comerford J, D’Orazio D, Dotti M, et al. (2019) Multi-Messenger Astrophysics With Pulsar Timing Arrays. BAAS 51(3):490. arXiv:1903.07644 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Kimpson T, Wu K, Zane S (2019a) Pulsar timing in extreme mass ratio binaries: a general relativistic approach. MNRAS 486(1):360–377. https://doi.org/10.1093/mnras/stz845 . arXiv:1903.08258 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Moody MSL, Shi JM, Stone JM (2019) Hydrodynamic Torques in Circumbinary Accretion Disks. ApJ 875(1):66. https://doi.org/10.3847/1538-4357/ab09ee . arXiv:1903.00008 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Mushotzky R, Aird J, Barger AJ, Cappelluti N, Chartas G, Corrales L, Eufrasio R, Fabian AC, Falcone AD, Gallo E, et al. (2019) The Advanced X-ray Imaging Satellite. In: Bulletin of the American Astronomical Society. vol 51. p 107. arXiv:1903.04083 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Pfister H, Bar-Or B, Volonteri M, Dubois Y, Capelo PR (2019a) Tidal disruption event rates in galaxy merger remnants. MNRAS 488(1):L29–L34. https://doi.org/10.1093/mnrasl/slz091 . arXiv:1903.09124 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Ray PS, Arzoumanian Z, Ballantyne D, Bozzo E, Brandt S, Brenneman L, Chakrabarty D, Christophersen M, DeRosa A, Feroci M, et al. (2019) STROBE-X: X-ray Timing and Spectroscopy on Dynamical Timescales from Microseconds to Years. arXiv e-prints arXiv:1903.03035. arXiv:1903.03035 [astro-ph.IM]

Original

1903

Earlier work this paper cites.

Reynolds CS (2019) Observing black holes spin. Nature Astronomy 3:41–47. https://doi.org/10.1038/s41550-018-0665-z . arXiv:1903.11704 [astro-ph.HE]

Original

1903

Earlier work this paper cites.

Sahu N, Graham AW, Davis BL (2019a) Black Hole Mass Scaling Relations for Early-type Galaxies. I. M BH

Original

1903

Earlier work this paper cites.

Saladino MI, Pols OR, Abate C (2019) Slowly, slowly in the wind. 3D hydrodynamical simulations of wind mass transfer and angular-momentum loss in AGB binary systems. A&A 626:A68. https://doi.org/10.1051/0004-6361/201834598 . arXiv:1903.04515 [astro-ph.SR]

Original

1903

Earlier work this paper cites.

Stephan AP, Naoz S, Ghez AM, Morris MR, Ciurlo A, Do T, Breivik K, Coughlin S, Rodriguez CL (2019) The Fate of Binaries in the Galactic Center: The Mundane and the Exotic. ApJ 878(1):58. https://doi.org/10.3847/1538-4357/ab1e4d . arXiv:1903.00010 [astro-ph.SR]

Original

1903

Earlier work this paper cites.

Taylor S, Burke-Spolaor S, Baker PT, Charisi M, Islo K, Kelley LZ, Madison DR, Simon J, Vigeland S, Nanograv Collaboration (2019) Supermassive Black-hole Demographics &Environments With Pulsar Timing Arrays. BAAS 51(3):336. arXiv:1903.08183 [astro-ph.GA]

Original

1903

Earlier work this paper cites.

Andrews JJ, Zezas A (2019) Double neutron star formation: merger times, systemic velocities, and travel distances. MNRAS 486(3):3213–3227. https://doi.org/10.1093/mnras/stz1066 . arXiv:1904.06137 [astro-ph.HE]

Original

1904

Earlier work this paper cites.

Bowen DB, Mewes V, Noble SC, Avara M, Campanelli M, Krolik JH (2019) Quasi-periodicity of Supermassive Binary Black Hole Accretion Approaching Merger. ApJ 879(2):76. https://doi.org/10.3847/1538-4357/ab2453 . arXiv:1904.12048 [astro-ph.HE]

Original

1904

Earlier work this paper cites.

Cromartie HT, Fonseca E, Ransom SM, Demorest PB, Arzoumanian Z, Blumer H, Brook PR, DeCesar ME, Dolch T, Ellis JA, et al. (2020) Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar. Nature Astronomy 4:72–76. https://doi.org/10.1038/s41550-019-0880-2 . arXiv:1904.06759 [astro-ph.HE]

Original

1904

Earlier work this paper cites.

Cusin G, Dvorkin I, Pitrou C, Uzan JP (2020) Stochastic gravitational wave background anisotropies in the mHz band: astrophysical dependencies. MNRAS 493(1):L1–L5. https://doi.org/10.1093/mnrasl/slz182 . arXiv:1904.07757 [astro-ph.CO]

Original

1904

Earlier work this paper cites.

Gaspari M, Eckert D, Ettori S, Tozzi P, Bassini L, Rasia E, Brighenti F, Sun M, Borgani S, Johnson SD, et al. (2019) The X-Ray Halo Scaling Relations of Supermassive Black Holes. ApJ 884(2):169. https://doi.org/10.3847/1538-4357/ab3c5d . arXiv:1904.10972 [astro-ph.GA]

Original

1904

Earlier work this paper cites.

Giersz M, Askar A, Wang L, Hypki A, Leveque A, Spurzem R (2019) MOCCA survey data base- I. Dissolution of tidally filling star clusters harbouring black hole subsystems. MNRAS 487(2):2412–2423. https://doi.org/10.1093/mnras/stz1460 . arXiv:1904.01227 [astro-ph.GA]

Original

1904

Earlier work this paper cites.

Jiang YF, Blaes O, Stone JM, Davis SW (2019) Global Radiation Magnetohydrodynamic Simulations of sub-Eddington Accretion Disks around Supermassive Black Holes. ApJ 885(2):144. https://doi.org/10.3847/1538-4357/ab4a00 . arXiv:1904.01674 [astro-ph.HE]

Original

1904

Earlier work this paper cites.

Manser CJ, Gänsicke BT, Eggl S, Hollands M, Izquierdo P, Koester D, Landstreet JD, Lyra W, Marsh TR, Meru F, et al. (2019) A planetesimal orbiting within the debris disc around a white dwarf star. Science 364(6435):66–69. https://doi.org/10.1126/science.aat5330 . arXiv:1904.02163 [astro-ph.EP]

Original

1904

Earlier work this paper cites.

Margalit B, Metzger BD (2019) The Multi-messenger Matrix: The Future of Neutron Star Merger Constraints on the Nuclear Equation of State. ApJ 880(1):L15. https://doi.org/10.3847/2041-8213/ab2ae2 . arXiv:1904.11995 [astro-ph.HE]

Original

1904

Earlier work this paper cites.

Prust LJ, Chang P (2019) Common envelope evolution on a moving mesh. MNRAS 486(4):5809–5818. https://doi.org/10.1093/mnras/stz1219 . arXiv:1904.09256 [astro-ph.SR]

Original

1904

Earlier work this paper cites.

Watts AL (2019) Constraining the neutron star equation of state using pulse profile modeling. In: Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy. American Institute of Physics Conference Series, vol 2127. p 020008. https://doi.org/10.1063/1.5117798 . arXiv:1904.07012 [astro-ph.HE]

Original

1904

Earlier work this paper cites.

Arca Sedda M, Askar A, Giersz M (2019a) MOCCA-SURVEY Database I. Intermediate mass black holes in Milky Way globular clusters and their connection to supermassive black holes. arXiv e-prints arXiv:1905.00902. arXiv:1905.00902 [astro-ph.GA]

Original

1905

Earlier work this paper cites.

Bonga B, Yang H, Hughes SA (2019) Tidal Resonance in Extreme Mass-Ratio Inspirals. Phys. Rev. Lett. 123(10):101103. https://doi.org/10.1103/PhysRevLett.123.101103 . arXiv:1905.00030 [gr-qc]

Original

1905

Earlier work this paper cites.

Carson Z, Yagi K (2020) Multi-band gravitational wave tests of general relativity. Classical and Quantum Gravity 37(2):02LT01. https://doi.org/10.1088/1361-6382/ab5c9a . arXiv:1905.13155 [gr-qc]

Original

1905

Earlier work this paper cites.

Gnocchi G, Maselli A, Abdelsalhin T, Giacobbo N, Mapelli M (2019) Bounding alternative theories of gravity with multiband GW observations. Phys. Rev. D 100(6):064024. https://doi.org/10.1103/PhysRevD.100.064024 . arXiv:1905.13460 [gr-qc]

Original

1905

Earlier work this paper cites.

Krolik JH, Volonteri M, Dubois Y, Devriendt J (2019) Population estimates for electromagnetically distinguishable supermassive binary black holes. ApJ 879(2):110. https://doi.org/10.3847/1538-4357/ab24c9 . arXiv:1905.10450 [astro-ph.GA]

Original

1905

Earlier work this paper cites.

Marinacci F, Sales LV, Vogelsberger M, Torrey P, Springel V (2019) Simulating the interstellar medium and stellar feedback on a moving mesh: implementation and isolated galaxies. MNRAS 489(3):4233–4260. https://doi.org/10.1093/mnras/stz2391 . arXiv:1905.08806 [astro-ph.GA]

Original

1905

Earlier work this paper cites.

Moore CJ, Gerosa D, Klein A (2019) Are stellar-mass black-hole binaries too quiet for LISA? MNRAS 488(1):L94–L98. https://doi.org/10.1093/mnrasl/slz104 . arXiv:1905.11998 [astro-ph.HE]

Original

1905

Earlier work this paper cites.

Akiyama K, Alberdi A, Alef W, Asada K, Azulay R, Baczko AK, Ball D, Baloković M, Barrett J, Bintley D, et al. (2019) First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole. ApJ 875(1):L1. https://doi.org/10.3847/2041-8213/ab0ec7 . arXiv:1906.11238 [astro-ph.GA]

Original

1906

Earlier work this paper cites.

Antonini F, Gieles M (2020) Population synthesis of black hole binary mergers from star clusters. MNRAS 492(2):2936–2954. https://doi.org/10.1093/mnras/stz3584 . arXiv:1906.11855 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Arca Sedda M, Mastrobuono-Battisti A (2019) Mergers of globular clusters in the Galactic disc: intermediate mass black hole coalescence and implications for gravitational waves detection. arXiv e-prints arXiv:1906.05864. arXiv:1906.05864 [astro-ph.GA]

Original

1906

Earlier work this paper cites.

Bavera SS, Fragos T, Qin Y, Zapartas E, Neijssel CJ, Mandel I, Batta A, Gaebel SM, Kimball C, Stevenson S (2020) The origin of spin in binary black holes. Predicting the distributions of the main observables of Advanced LIGO. A&A 635:A97. https://doi.org/10.1051/0004-6361/201936204 . arXiv:1906.12257 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Caprini C, Figueroa DG, Flauger R, Nardini G, Peloso M, Pieroni M, Ricciardone A, Tasinato G (2019) Reconstructing the spectral shape of a stochastic gravitational wave background with LISA. J. Cosmology Astropart. Phys. 2019(11):017. https://doi.org/10.1088/1475-7516/2019/11/017 . arXiv:1906.09244 [astro-ph.CO]

Original

1906

Earlier work this paper cites.

DeGraf C, Sijacki D (2020) Cosmological simulations of massive black hole seeds: predictions for next-generation electromagnetic and gravitational wave observations. MNRAS 491(4):4973–4992. https://doi.org/10.1093/mnras/stz3309 . arXiv:1906.11271 [astro-ph.GA]

Original

1906

Earlier work this paper cites.

Event Horizon Telescope Collaboration, Akiyama K, Alberdi A, Alef W, Asada K, Azulay R, Baczko AK, Ball D, Baloković M, Barrett J, et al. (2019) First M87 Event Horizon Telescope Results. II. Array and Instrumentation. ApJ 875(1):L2. https://doi.org/10.3847/2041-8213/ab0c96 . arXiv:1906.11239 [astro-ph.IM]

Original

1906

Earlier work this paper cites.

Fluri J, Kacprzak T, Lucchi A, Refregier A, Amara A, Hofmann T, Schneider A (2019) Cosmological constraints with deep learning from KiDS-450 weak lensing maps. Phys. Rev. D 100(6):063514. https://doi.org/10.1103/PhysRevD.100.063514 . arXiv:1906.03156 [astro-ph.CO]

Original

1906

Earlier work this paper cites.

Gruzinov A, Levin Y, Matzner CD (2020) Negative dynamical friction on compact objects moving through dense gas. MNRAS 492(2):2755–2761. https://doi.org/10.1093/mnras/staa013 . arXiv:1906.01186 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Hannuksela OA, Ng KCY, Li TGF (2020) Extreme dark matter tests with extreme mass ratio inspirals. Phys. Rev. D 102(10):103022. https://doi.org/10.1103/PhysRevD.102.103022 . arXiv:1906.11845 [astro-ph.CO]

Original

1906

Earlier work this paper cites.

Karnesis N, Lilley M, Petiteau A (2019) Assessing the detectability of a Stochastic Gravitational Wave Background with LISA, using an excess of power approach. arXiv e-prints arXiv:1906.09027. arXiv:1906.09027 [astro-ph.IM]

Original

1906

Earlier work this paper cites.

Liu T, Gezari S, Ayers M, Burgett W, Chambers K, Hodapp K, Huber ME, Kudritzki RP, Metcalfe N, Tonry J, et al. (2019b) Supermassive Black Hole Binary Candidates from the Pan-STARRS1 Medium Deep Survey. ApJ 884(1):36. https://doi.org/10.3847/1538-4357/ab40cb . arXiv:1906.08315 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Napiwotzki R, Karl CA, Lisker T, Catalán S, Drechsel H, Heber U, Homeier D, Koester D, Leibundgut B, Marsh TR, et al. (2020) The ESO supernovae type Ia progenitor survey (SPY). The radial velocities of 643 DA white dwarfs. A&A 638:A131. https://doi.org/10.1051/0004-6361/201629648 . arXiv:1906.10977 [astro-ph.SR]

Original

1906

Earlier work this paper cites.

Neijssel CJ, Vigna-Gómez A, Stevenson S, Barrett JW, Gaebel SM, Broekgaarden FS, de Mink SE, Szécsi D, Vinciguerra S, Mandel I (2019) The effect of the metallicity-specific star formation history on double compact object mergers. MNRAS 490(3):3740–3759. https://doi.org/10.1093/mnras/stz2840 . arXiv:1906.08136 [astro-ph.SR]

Original

1906

Earlier work this paper cites.

Rodriguez CL, Zevin M, Amaro-Seoane P, Chatterjee S, Kremer K, Rasio FA, Ye CS (2019) Black holes: The next generation—repeated mergers in dense star clusters and their gravitational-wave properties. Phys. Rev. D 100(4):043027. https://doi.org/10.1103/PhysRevD.100.043027 . arXiv:1906.10260 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Vick M, Lai D (2019) Tidal effects in eccentric coalescing neutron star binaries. Phys. Rev. D 100(6):063001. https://doi.org/10.1103/PhysRevD.100.063001 . arXiv:1906.08780 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Yang Y, Bartos I, Gayathri V, Ford KES, Haiman Z, Klimenko S, Kocsis B, Márka S, Márka Z, McKernan B, et al. (2019) Hierarchical Black Hole Mergers in Active Galactic Nuclei. Phys. Rev. Lett. 123(18):181101. https://doi.org/10.1103/PhysRevLett.123.181101 . arXiv:1906.09281 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Zevin M, Kremer K, Siegel DM, Coughlin S, Tsang BTH, Berry CPL, Kalogera V (2019a) Can Neutron-star Mergers Explain the r-process Enrichment in Globular Clusters? ApJ 886(1):4. https://doi.org/10.3847/1538-4357/ab498b . arXiv:1906.11299 [astro-ph.HE]

Original

1906

Earlier work this paper cites.

Baghi Q, Thorpe JI, Slutsky J, Baker J, Canton TD, Korsakova N, Karnesis N (2019) Gravitational-wave parameter estimation with gaps in LISA: A Bayesian data augmentation method. Phys. Rev. D 100(2):022003. https://doi.org/10.1103/PhysRevD.100.022003 . arXiv:1907.04747 [gr-qc]

Original

1907

Earlier work this paper cites.

Boco L, Lapi A, Goswami S, Perrotta F, Baccigalupi C, Danese L (2019) Merging Rates of Compact Binaries in Galaxies: Perspectives for Gravitational Wave Detections. ApJ 881(2):157. https://doi.org/10.3847/1538-4357/ab328e . arXiv:1907.06841 [astro-ph.GA]

Original

1907

Earlier work this paper cites.

Burdge KB, Coughlin MW, Fuller J, Kupfer T, Bellm EC, Bildsten L, Graham MJ, et al (2019a) General relativistic orbital decay in a seven-minute-orbital-period eclipsing binary system. Nature 571(7766):528–531. https://doi.org/10.1038/s41586-019-1403-0 . arXiv:1907.11291 [astro-ph.SR]

Original

1907

Earlier work this paper cites.

Chruslinska M, Nelemans G (2019) Metallicity of stars formed throughout the cosmic history based on the observational properties of star-forming galaxies. MNRAS 488(4):5300–5326. https://doi.org/10.1093/mnras/stz2057 . arXiv:1907.11243 [astro-ph.GA]

Original

1907

Earlier work this paper cites.

Copperwheat CM, Marsh TR, Littlefair SP, Dhillon VS, Ramsay G, Drake AJ, Gänsicke BT, Groot PJ, Hakala P, Koester D, et al. (2011) SDSS J0926+3624: the shortest period eclipsing binary star. MNRAS 410(2):1113–1129. https://doi.org/10.1111/j.1365-2966.2010.17508.x . arXiv:1008.1907 [astro-ph.SR]

Original

1907

Earlier work this paper cites.

Fragos T, Andrews JJ, Ramirez-Ruiz E, Meynet G, Kalogera V, Taam RE, Zezas A (2019) The Complete Evolution of a Neutron-star Binary through a Common Envelope Phase Using 1D Hydrodynamic Simulations. ApJ 883(2):L45. https://doi.org/10.3847/2041-8213/ab40d1 . arXiv:1907.12573 [astro-ph.HE]

Original

1907

Earlier work this paper cites.

Hamilton C, Rafikov RR (2019a) Compact Object Binary Mergers Driven By Cluster Tides: A New Channel for LIGO/Virgo Gravitational-wave Events. ApJ 881(1):L13. https://doi.org/10.3847/2041-8213/ab3468 . arXiv:1907.00994 [astro-ph.GA]

Original

1907

Earlier work this paper cites.

Inman D, Ali-Haïmoud Y (2019) Early structure formation in primordial black hole cosmologies. Phys Rev D 100(8):083528. https://doi.org/10.1103/PhysRevD.100.083528 . arXiv:1907.08129 [astro-ph.CO]

Original

1907

Earlier work this paper cites.

Lamberts A, Blunt S, Littenberg TB, Garrison-Kimmel S, Kupfer T, Sanderson RE (2019) Predicting the LISA white dwarf binary population in the Milky Way with cosmological simulations. MNRAS 490(4):5888–5903. https://doi.org/10.1093/mnras/stz2834 . arXiv:1907.00014 [astro-ph.HE]

Original

1907

Earlier work this paper cites.

McKernan B, Ford KES, Bartos I, Graham MJ, Lyra W, Marka S, Marka Z, Ross NP, Stern D, Yang Y (2019) Ram-pressure Stripping of a Kicked Hill Sphere: Prompt Electromagnetic Emission from the Merger of Stellar Mass Black Holes in an AGN Accretion Disk. ApJ 884(2):L50. https://doi.org/10.3847/2041-8213/ab4886 . arXiv:1907.03746 [astro-ph.HE]

Original

1907

Earlier work this paper cites.

McKernan B, Ford KES, O’Shaugnessy R, Wysocki D (2020b) Monte Carlo simulations of black hole mergers in AGN discs: Low χ \chi eff

Original

1907

Earlier work this paper cites.

Randall L, Xianyu ZZ (2019a) Eccentricity Without Measuring Eccentricity: Discriminating Among Stellar Mass Black Hole Binary Formation Channels. arXiv e-prints arXiv:1907.02283. arXiv:1907.02283 [astro-ph.HE]

Original

1907

Earlier work this paper cites.

Tamanini N, Klein A, Bonvin C, Barausse E, Caprini C (2020) Peculiar acceleration of stellar-origin black hole binaries: Measurement and biases with LISA. Phys. Rev. D 101(6):063002. https://doi.org/10.1103/PhysRevD.101.063002 . arXiv:1907.02018 [astro-ph.IM]

Original

1907

Earlier work this paper cites.

Arca Sedda M, Berry CPL, Jani K, Amaro-Seoane P, Auclair P, Baird J, Baker T, Berti E, Breivik K, Burrows A, et al. (2020a) The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range. Classical and Quantum Gravity 37(21):215011. https://doi.org/10.1088/1361-6382/abb5c1 . arXiv:1908.11375 [gr-qc]

Original

1908

Earlier work this paper cites.

Euclid Collaboration, Barnett R, Warren SJ, Mortlock DJ, Cuby JG, Conselice C, Hewett PC, Willott CJ, Auricchio N, Balaguera-Antolínez A, et al. (2019) Euclid preparation. V. Predicted yield of redshift 7 < z < 9 quasars from the wide survey. A&A 631:A85. https://doi.org/10.1051/0004-6361/201936427 . arXiv:1908.04310 [astro-ph.GA]

Original

1908

Earlier work this paper cites.

Gänsicke BT, Marsh TR, Southworth J, Rebassa-Mansergas A (2006) A Gaseous Metal Disk Around a White Dwarf. Science 314(5807):1908. https://doi.org/10.1126/science.1135033 . arXiv:astro-ph/0612697 [astro-ph]

1908

Earlier work this paper cites.

Jani K, Shoemaker D, Cutler C (2019) Detectability of intermediate-mass black holes in multiband gravitational wave astronomy. Nature Astronomy 4:260–265. https://doi.org/10.1038/s41550-019-0932-7 . arXiv:1908.04985 [gr-qc]

Original

1908

Earlier work this paper cites.

Jha SW, Maguire K, Sullivan M (2019) Observational properties of thermonuclear supernovae. Nature Astronomy 3:706–716. https://doi.org/10.1038/s41550-019-0858-0 . arXiv:1908.02303 [astro-ph.HE]

Original

1908

Earlier work this paper cites.

Kalaja A, Bellomo N, Bartolo N, Bertacca D, Matarrese S, Musco I, Raccanelli A, Verde L (2019) From Primordial Black Holes Abundance to Primordial Curvature Power Spectrum (and back). JCAP 10:031. https://doi.org/10.1088/1475-7516/2019/10/031 . arXiv:1908.03596 [astro-ph.CO]

Original

1908

Earlier work this paper cites.

Katz ML, Kelley LZ, Dosopoulou F, Berry S, Blecha L, Larson SL (2020) Probing massive black hole binary populations with LISA. MNRAS 491(2):2301–2317. https://doi.org/10.1093/mnras/stz3102 . arXiv:1908.05779 [astro-ph.HE]

Original

1908

Earlier work this paper cites.

Littenberg TB, Cornish NJ (2019) Prospects for Gravitational Wave Measurement of ZTF J1539+5027. ApJ 881(2):L43. https://doi.org/10.3847/2041-8213/ab385f . arXiv:1908.00678 [astro-ph.IM]

Original

1908

Earlier work this paper cites.

Matsuoka Y, Iwasawa K, Onoue M, Kashikawa N, Strauss MA, Lee CH, Imanishi M, Nagao T, Akiyama M, Asami N, et al. (2019) Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 ≤ \leq z ≤ \leq 7.0. ApJ 883(2):183. https://doi.org/10.3847/1538-4357/ab3c60 . arXiv:1908.07910 [astro-ph.GA]

Original

1908

Earlier work this paper cites.

Nguyen K, Bogdanović T, Runnoe JC, Eracleous M, Sigurdsson S, Boroson T (2020) Emission Signatures from Subparsec Binary Supermassive Black Holes. III. Comparison of Models with Observations. ApJ 894(2):105. https://doi.org/10.3847/1538-4357/ab88b5 . arXiv:1908.01799 [astro-ph.HE]

Original

1908

Earlier work this paper cites.

Pound A, Wardell B, Warburton N, Miller J (2020) Second-Order Self-Force Calculation of Gravitational Binding Energy in Compact Binaries. Phys. Rev. Lett. 124(2):021101. https://doi.org/10.1103/PhysRevLett.124.021101 . arXiv:1908.07419 [gr-qc]

Original

1908

Earlier work this paper cites.

Ransom S, Brazier A, Chatterjee S, Cohen T, Cordes JM, DeCesar ME, Demorest PB, Hazboun JS, Lam MT, Lynch RS, et al. (2019) The NANOGrav Program for Gravitational Waves and Fundamental Physics. In: Bulletin of the American Astronomical Society. vol 51. p 195. arXiv:1908.05356 [astro-ph.IM]

Original

1908

Earlier work this paper cites.

Regan JA, Wise JH, O’Shea BW, Norman ML (2020b) The emergence of the first star-free atomic cooling haloes in the Universe. MNRAS 492(2):3021–3031. https://doi.org/10.1093/mnras/staa035 . arXiv:1908.02823 [astro-ph.GA]

Original

1908

Earlier work this paper cites.

Sahu N, Graham AW, Davis BL (2019b) Revealing Hidden Substructures in the M BH

Original

1908

Earlier work this paper cites.

Sesana A, Korsakova N, Arca Sedda M, Baibhav V, Barausse E, Barke S, Berti E, Bonetti M, Capelo PR, Caprini C, et al. (2021) Unveiling the gravitational universe at μ \mu -Hz frequencies. Experimental Astronomy 51(3):1333–1383. https://doi.org/10.1007/s10686-021-09709-9 . arXiv:1908.11391 [astro-ph.IM]

Original

1908

Earlier work this paper cites.

Smith TL, Caldwell RR (2019) LISA for cosmologists: Calculating the signal-to-noise ratio for stochastic and deterministic sources. Phys. Rev. D 100(10):104055. https://doi.org/10.1103/PhysRevD.100.104055 . arXiv:1908.00546 [astro-ph.CO]

Original

1908

Earlier work this paper cites.

Toscani M, Lodato G, Nealon R (2019) Gravitational wave emission from unstable accretion discs in tidal disruption events. MNRAS 489(1):699–706. https://doi.org/10.1093/mnras/stz2201 . arXiv:1908.02969 [astro-ph.HE]

Original

1908

Earlier work this paper cites.

Bañados E, Novak M, Neeleman M, Walter F, Decarli R, Venemans BP, Mazzucchelli C, Carilli C, Wang F, Fan X, et al. (2019) The z = 7.54 Quasar ULAS J1342+0928 Is Hosted by a Galaxy Merger. ApJ 881(1):L23. https://doi.org/10.3847/2041-8213/ab3659 . arXiv:1909.00027 [astro-ph.GA]

Original

1909

Earlier work this paper cites.

Cardoso V, Maselli A (2020) Constraints on the astrophysical environment of binaries with gravitational-wave observations. A&A 644:A147. https://doi.org/10.1051/0004-6361/202037654 . arXiv:1909.05870 [astro-ph.HE]

Original

1909

Earlier work this paper cites.

Chua AJK, Vallisneri M (2020) Learning Bayesian Posteriors with Neural Networks for Gravitational-Wave Inference. Phys. Rev. Lett. 124(4):041102. https://doi.org/10.1103/PhysRevLett.124.041102 . arXiv:1909.05966 [gr-qc]

Original

1909

Earlier work this paper cites.

Dage KC, Zepf SE, Bahramian A, Strader J, Maccarone TJ, Peacock MB, Kundu A, Steele MM, Britt CT (2019) Slow decline and rise of the broad [O III] emission line in globular cluster black hole candidate RZ2109. MNRAS 489(4):4783–4790. https://doi.org/10.1093/mnras/stz2514 . arXiv:1909.02683 [astro-ph.HE]

Original

1909

Earlier work this paper cites.

Deme B, Meiron Y, Kocsis B (2020b) Intermediate-mass Black Holes’ Effects on Compact Object Binaries. ApJ 892(2):130. https://doi.org/10.3847/1538-4357/ab7921 . arXiv:1909.04678 [astro-ph.GA]

Original

1909

Earlier work this paper cites.

Giacobbo N, Mapelli M (2020) Revising Natal Kick Prescriptions in Population Synthesis Simulations. ApJ 891(2):141. https://doi.org/10.3847/1538-4357/ab7335 . arXiv:1909.06385 [astro-ph.HE]

Original

1909

Earlier work this paper cites.

Johnson M, Haworth K, Pesce DW, Palumbo DCM, Blackburn L, Akiyama K, Boroson D, Bouman KL, Farah JR, Fish VL, et al. (2019) Studying black holes on horizon scales with space-VLBI. In: Bulletin of the American Astronomical Society. vol 51. p 235. arXiv:1909.01405 [astro-ph.IM]

Original

1909

Earlier work this paper cites.

MacLeod M, Lin DNC (2020) The Effect of Star-Disk Interactions on Highly Eccentric Stellar Orbits in Active Galactic Nuclei: A Disk Loss Cone and Implications for Stellar Tidal Disruption Events. ApJ 889(2):94. https://doi.org/10.3847/1538-4357/ab64db . arXiv:1909.09645 [astro-ph.SR]

Original

1909

Earlier work this paper cites.

Mannerkoski M, Johansson PH, Pihajoki P, Rantala A, Naab T (2019) Gravitational Waves from the Inspiral of Supermassive Black Holes in Galactic-scale Simulations. ApJ 887(1):35. https://doi.org/10.3847/1538-4357/ab52f9 . arXiv:1909.01373 [astro-ph.GA]

Original

1909

Earlier work this paper cites.

Obergaulinger M, Aloy MÁ (2020) Magnetorotational core collapse of possible GRB progenitors - I. Explosion mechanisms. MNRAS 492(4):4613–4634. https://doi.org/10.1093/mnras/staa096 . arXiv:1909.01105 [astro-ph.HE]

Original

1909

Earlier work this paper cites.

Perera BBP, DeCesar ME, Demorest PB, Kerr M, Lentati L, Nice DJ, Osłowski S, Ransom SM, Keith MJ, Arzoumanian Z, et al. (2019) The International Pulsar Timing Array: second data release. MNRAS 490(4):4666–4687. https://doi.org/10.1093/mnras/stz2857 . arXiv:1909.04534 [astro-ph.HE]

Original

1909

Earlier work this paper cites.

Reines AE, Condon JJ, Darling J, Greene JE (2020) A New Sample of (Wandering) Massive Black Holes in Dwarf Galaxies from High-resolution Radio Observations. ApJ 888(1):36. https://doi.org/10.3847/1538-4357/ab4999 . arXiv:1909.04670 [astro-ph.GA]

Original

1909

Earlier work this paper cites.

Romero-Shaw IM, Lasky PD, Thrane E (2019) Searching for eccentricity: signatures of dynamical formation in the first gravitational-wave transient catalogue of LIGO and Virgo. MNRAS 490(4):5210–5216. https://doi.org/10.1093/mnras/stz2996 . arXiv:1909.05466 [astro-ph.HE]

Original

1909

Earlier work this paper cites.

Seto N (2019) Search for neutron star binaries in the Local Group galaxies using LISA. MNRAS 489(4):4513–4519. https://doi.org/10.1093/mnras/stz2439 . arXiv:1909.01471 [astro-ph.HE]

Original

1909

Earlier work this paper cites.

Stephan AP, Naoz S, Gaudi BS, Salas JM (2020) Eating Planets for Lunch and Dinner: Signatures of Planet Consumption by Evolving Stars. ApJ 889(1):45. https://doi.org/10.3847/1538-4357/ab5b00 . arXiv:1909.05259 [astro-ph.SR]

Original

1909

Earlier work this paper cites.

Tagawa H, Haiman Z, Kocsis B (2020b) Making a Supermassive Star by Stellar Bombardment. ApJ 892(1):36. https://doi.org/10.3847/1538-4357/ab7922 . arXiv:1909.10517 [astro-ph.GA]

Original

1909

Earlier work this paper cites.

Andrews JJ, Breivik K, Pankow C, D’Orazio DJ, Safarzadeh M (2020) LISA and the Existence of a Fast-merging Double Neutron Star Formation Channel. ApJ 892(1):L9. https://doi.org/10.3847/2041-8213/ab5b9a . arXiv:1910.13436 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Burdge KB, Fuller J, Phinney ES, van Roestel J, Claret A, Cukanovaite E, Gentile Fusillo NP, Coughlin MW, Kaplan DL, Kupfer T, et al. (2019b) Orbital Decay in a 20 Minute Orbital Period Detached Binary with a Hydrogen-poor Low-mass White Dwarf. ApJ 886(1):L12. https://doi.org/10.3847/2041-8213/ab53e5 . arXiv:1910.11389 [astro-ph.SR]

Original

1910

Earlier work this paper cites.

Comerford TAF, Izzard RG, Booth RA, Rosotti G (2019) Bondi-Hoyle-Lyttleton accretion by binary stars. MNRAS 490(4):5196–5209. https://doi.org/10.1093/mnras/stz2977 . arXiv:1910.13353 [astro-ph.SR]

Original

1910

Earlier work this paper cites.

Danielski C, Korol V, Tamanini N, Rossi EM (2019) Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna. A&A 632:A113. https://doi.org/10.1051/0004-6361/201936729 . arXiv:1910.05414 [astro-ph.EP]

Original

1910

Earlier work this paper cites.

De S, MacLeod M, Everson RW, Antoni A, Mandel I, Ramirez-Ruiz E (2020) Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-driven Growth of LIGO Binary Black Holes. ApJ 897(2):130. https://doi.org/10.3847/1538-4357/ab9ac6 . arXiv:1910.13333 [astro-ph.SR]

Original

1910

Earlier work this paper cites.

Dullo BT (2019) The Most Massive Galaxies with Large Depleted Cores: Structural Parameter Relations and Black Hole Masses. ApJ 886(2):80. https://doi.org/10.3847/1538-4357/ab4d4f . arXiv:1910.10240 [astro-ph.GA]

Original

1910

Earlier work this paper cites.

Farmer R, Renzo M, de Mink SE, Marchant P, Justham S (2019) Mind the Gap: The Location of the Lower Edge of the Pair-instability Supernova Black Hole Mass Gap. ApJ 887(1):53. https://doi.org/10.3847/1538-4357/ab518b . arXiv:1910.12874 [astro-ph.SR]

Original

1910

Earlier work this paper cites.

Hu BX, D’Orazio DJ, Haiman Z, Smith KL, Snios B, Charisi M, Di Stefano R (2020) Spikey: self-lensing flares from eccentric SMBH binaries. MNRAS 495(4):4061–4070. https://doi.org/10.1093/mnras/staa1312 . arXiv:1910.05348 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Kawka A, Vennes S, Ferrario L (2020) An ancient double degenerate merger in the Milky Way halo. MNRAS 491(1):L40–L45. https://doi.org/10.1093/mnrasl/slz165 . arXiv:1910.13053 [astro-ph.SR]

Original

1910

Earlier work this paper cites.

Korol V, Rossi EM, Groot PJ, Nelemans G, Toonen S, Brown AGA (2017) Prospects for detection of detached double white dwarf binaries with Gaia, LSST and LISA. MNRAS 470(2):1894–1910. https://doi.org/10.1093/mnras/stx1285 . arXiv:1703.02555 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Lau MYM, Mandel I, Vigna-Gómez A, Neijssel CJ, Stevenson S, Sesana A (2020) Detecting double neutron stars with LISA. MNRAS 492(3):3061–3072. https://doi.org/10.1093/mnras/staa002 . arXiv:1910.12422 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Metzger BD (2019) Kilonovae. Living Reviews in Relativity 23(1):1. https://doi.org/10.1007/s41114-019-0024-0 . arXiv:1910.01617 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Muñoz DJ, Lai D, Kratter K, Mirand a R (2020) Circumbinary Accretion from Finite and Infinite Disks. ApJ 889(2):114. https://doi.org/10.3847/1538-4357/ab5d33 . arXiv:1910.04763 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Thrane E, Osłowski S, Lasky PD (2020) Ultrarelativistic astrophysics using multimessenger observations of double neutron stars with LISA and the SKA. MNRAS 493(4):5408–5412. https://doi.org/10.1093/mnras/staa593 . arXiv:1910.12330 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Tsizh M, Novosyadlyj B, Holovatch Y, Libeskind NI (2020) Large-scale structures in the Λ \Lambda CDM Universe: network analysis and machine learning. MNRAS 495(1):1311–1320. https://doi.org/10.1093/mnras/staa1030 . arXiv:1910.07868 [astro-ph.CO]

Original

1910

Earlier work this paper cites.

von Zeipel H (1910) Sur l’application des séries de M. Lindstedt à l’étude du mouvement des comètes périodiques. Astronomische Nachrichten 183(22):345. https://doi.org/10.1002/asna.19091832202

1910

Earlier work this paper cites.

Ye CS, Fong Wf, Kremer K, Rodriguez CL, Chatterjee S, Fragione G, Rasio FA (2020) On the Rate of Neutron Star Binary Mergers from Globular Clusters. ApJ 888(1):L10. https://doi.org/10.3847/2041-8213/ab5dc5 . arXiv:1910.10740 [astro-ph.HE]

Original

1910

Earlier work this paper cites.

Breivik K, Coughlin S, Zevin M, Rodriguez CL, Kremer K, Ye CS, Andrews JJ, Kurkowski M, Digman MC, Larson SL, et al. (2020a) COSMIC Variance in Binary Population Synthesis. ApJ 898(1):71. https://doi.org/10.3847/1538-4357/ab9d85 . arXiv:1911.00903 [astro-ph.HE]

Original

1911

Earlier work this paper cites.

Chamandy L, Frank A, Blackman EG, Carroll-Nellenback J, Liu B, Tu Y, Nordhaus J, Chen Z, Peng B (2018) Accretion in common envelope evolution. MNRAS 480(2):1898–1911. https://doi.org/10.1093/mnras/sty1950 . arXiv:1805.03607 [astro-ph.SR]

Original

1911

Earlier work this paper cites.

Di Carlo UN, Mapelli M, Bouffanais Y, Giacobbo N, Santoliquido F, Bressan Ar, Spera M, Haardt F (2020a) Binary black holes in the pair instability mass gap. MNRAS 497(1):1043–1049. https://doi.org/10.1093/mnras/staa1997 . arXiv:1911.01434 [astro-ph.HE]

Original

1911

Earlier work this paper cites.

Dittmann AJ, Miller MC (2020) Star formation in accretion discs and SMBH growth. MNRAS 493(3):3732–3743. https://doi.org/10.1093/mnras/staa463 . arXiv:1911.08685 [astro-ph.HE]

Original

1911

Earlier work this paper cites.

Duffell PC, D’Orazio D, Derdzinski A, Haiman Z, MacFadyen A, Rosen AL, Zrake J (2019) Circumbinary Disks: Accretion and Torque as a Function of Mass Ratio and Disk Viscosity. arXiv e-prints arXiv:1911.05506. arXiv:1911.05506 [astro-ph.SR]

Original

1911

Earlier work this paper cites.

Greene JE, Strader J, Ho LC (2019) Intermediate-Mass Black Holes. arXiv e-prints arXiv:1911.09678. arXiv:1911.09678 [astro-ph.GA]

Original

1911

Earlier work this paper cites.

Inayoshi K, Visbal E, Haiman Z (2019) The Assembly of the First Massive Black Holes. arXiv e-prints arXiv:1911.05791. arXiv:1911.05791 [astro-ph.GA]

Original

1911

Earlier work this paper cites.

Khan FM, Mirza MA, Holley-Bockelmann K (2020) Inward bound: the incredible journey of massive black holes as they pair and merge - I. The effect of mass ratio in flattened rotating galactic nuclei. MNRAS 492(1):256–267. https://doi.org/10.1093/mnras/stz3360 . arXiv:1911.07946 [astro-ph.GA]

Original

1911

Earlier work this paper cites.

Kremer K, Ye CS, Rui NZ, Weatherford NC, Chatterjee S, Fragione G, Rodriguez CL, Spera M, Rasio FA (2020b) Modeling Dense Star Clusters in the Milky Way and Beyond with the CMC Cluster Catalog. ApJS 247(2):48. https://doi.org/10.3847/1538-4365/ab7919 . arXiv:1911.00018 [astro-ph.HE]

Original

1911

Earlier work this paper cites.

Leung GYC, Leaman R, van de Ven G, Battaglia G (2020) A dwarf-dwarf merger and dark matter core as a solution to the globular cluster problems in the Fornax dSph. MNRAS 493(1):320–336. https://doi.org/10.1093/mnras/stz3017 . arXiv:1911.09167 [astro-ph.GA]

Original

1911

Earlier work this paper cites.

Liu J, Zhang H, Howard AW, Bai Z, Lu Y, Soria R, Justham S, Li X, Zheng Z, (2019a) A wide star-black-hole binary system from radial-velocity measurements. Nature 575(7784):618–621. https://doi.org/10.1038/s41586-019-1766-2 . arXiv:1911.11989 [astro-ph.SR]

Original

1911

Earlier work this paper cites.

Ogiya G, Hahn O, Mingarelli CMF, Volonteri M (2020) Accelerated orbital decay of supermassive black hole binaries in merging nuclear star clusters. MNRAS 493(3):3676–3689. https://doi.org/10.1093/mnras/staa444 . arXiv:1911.11526 [astro-ph.GA]

Original

1911

Earlier work this paper cites.

Safarzadeh M, Hamers AS, Loeb A, Berger E (2020a) Formation and Merging of Mass Gap Black Holes in Gravitational-wave Merger Events from Wide Hierarchical Quadruple Systems. ApJ 888(1):L3. https://doi.org/10.3847/2041-8213/ab5dc8 . arXiv:1911.04495 [astro-ph.HE]

Original

1911

Earlier work this paper cites.

Zelenka O, Lukes-Gerakopoulos G, Witzany V, Kopáček O (2020) Growth of resonances and chaos for a spinning test particle in the Schwarzschild background. Phys. Rev. D 101(2):024037. https://doi.org/10.1103/PhysRevD.101.024037 . arXiv:1911.00414 [gr-qc]

Original

1911

Earlier work this paper cites.

Zwick L, Capelo PR, Bortolas E, Mayer L, Amaro-Seoane P (2020) Improved gravitational radiation time-scales: significance for LISA and LIGO-Virgo sources. MNRAS 495(2):2321–2331. https://doi.org/10.1093/mnras/staa1314 . arXiv:1911.06024 [astro-ph.GA]

Original

1911

Earlier work this paper cites.

Breivik K, Mingarelli CMF, Larson SL (2020b) Constraining Galactic Structure with the LISA White Dwarf Foreground. ApJ 901(1):4. https://doi.org/10.3847/1538-4357/abab99 . arXiv:1912.02200 [astro-ph.GA]

Original

1912

Earlier work this paper cites.

Gänsicke BT, Schreiber MR, Toloza O, Gentile Fusillo NP, Koester D, Manser CJ (2019) Accretion of a giant planet onto a white dwarf star. Nature 576(7785):61–64. https://doi.org/10.1038/s41586-019-1789-8 . arXiv:1912.01611 [astro-ph.EP]

Original

1912

Earlier work this paper cites.

Howitt G, Stevenson S, Vigna-Gómez Ar, Justham S, Ivanova N, Woods TE, Neijssel CJ, Mandel I (2020) Luminous Red Novae: population models and future prospects. MNRAS 492(3):3229–3240. https://doi.org/10.1093/mnras/stz3542 . arXiv:1912.07771 [astro-ph.HE]

Original

1912

Earlier work this paper cites.

Miller MC, Lamb FK, Dittmann AJ, Bogdanov S, Arzoumanian Z, Gendreau KC, Guillot S, Harding AK, Ho WCG, Lattimer JM, et al. (2019) PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter. ApJ 887(1):L24. https://doi.org/10.3847/2041-8213/ab50c5 . arXiv:1912.05705 [astro-ph.HE]

Original

1912

Earlier work this paper cites.

Naoz S, Will CM, Ramirez-Ruiz E, Hees A, Ghez AM, Do T (2020) A Hidden Friend for the Galactic Center Black Hole, Sgr A*. ApJ 888(1):L8. https://doi.org/10.3847/2041-8213/ab5e3b . arXiv:1912.04910 [astro-ph.GA]

Original

1912

Earlier work this paper cites.

Raaijmakers G, Greif SK, Riley TE, Hinderer T, Hebeler K, Schwenk A, Watts AL, Nissanke S, Guillot S, Lattimer JM, et al. (2020) Constraining the Dense Matter Equation of State with Joint Analysis of NICER and LIGO/Virgo Measurements. ApJ 893(1):L21. https://doi.org/10.3847/2041-8213/ab822f . arXiv:1912.11031 [astro-ph.HE]

Original

1912

Earlier work this paper cites.

Riley TE, Watts AL, Bogdanov S, Ray PS, Ludlam RM, Guillot S, Arzoumanian Z, Baker CL, Bilous AV, Chakrabarty D, et al. (2019) A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation. ApJ 887(1):L21. https://doi.org/10.3847/2041-8213/ab481c . arXiv:1912.05702 [astro-ph.HE]

Original

1912

Earlier work this paper cites.

Sesana A, Lamberts A, Petiteau A (2020) Finding binary black holes in the Milky Way with LISA. MNRAS 494(1):L75–L80. https://doi.org/10.1093/mnrasl/slaa039 . arXiv:1912.07627 [astro-ph.GA]

Original

1912

Earlier work this paper cites.

Tagawa H, Haiman Z, Kocsis B (2020a) Formation and Evolution of Compact-object Binaries in AGN Disks. ApJ 898(1):25. https://doi.org/10.3847/1538-4357/ab9b8c . arXiv:1912.08218 [astro-ph.GA]

Original

1912

Earlier work this paper cites.

Flanagan ÉÉ, Hinderer T (2008) Constraining neutron-star tidal Love numbers with gravitational-wave detectors. Phys. Rev. D 77(2):021502. https://doi.org/10.1103/PhysRevD.77.021502 . arXiv:0709.1915 [astro-ph]

Original

1915

Earlier work this paper cites.

Lousto CO, Zlochower Y, Dotti M, Volonteri M (2012) Gravitational recoil from accretion-aligned black-hole binaries. Phys. Rev. D 85(8):084015. https://doi.org/10.1103/PhysRevD.85.084015 . arXiv:1201.1923 [gr-qc]

Original

1923

Earlier work this paper cites.

Hoyle F, Lyttleton RA (1939) The effect of interstellar matter on climatic variation. Proceedings of the Cambridge Philosophical Society 35(3):405. https://doi.org/10.1017/S0305004100021150

1939

Earlier work this paper cites.

Chandrasekhar S (1943) Dynamical Friction. I. General Considerations: the Coefficient of Dynamical Friction. ApJ 97:255. https://doi.org/10.1086/144517

1943

Earlier work this paper cites.

Bondi H, Hoyle F (1944) On the mechanism of accretion by stars. MNRAS 104:273. https://doi.org/10.1093/mnras/104.5.273

1944

Earlier work this paper cites.

Alexander DM, Hickox RC (2012) What drives the growth of black holes? New A Rev. 56(4):93–121. https://doi.org/10.1016/j.newar.2011.11.003 . arXiv:1112.1949 [astro-ph.GA]

Original

1949

Earlier work this paper cites.

Kruckow MU, Tauris TM, Langer N, Kramer M, Izzard RG (2018) Progenitors of gravitational wave mergers: binary evolution with the stellar grid-based code COMBINE. MNRAS 481(2):1908–1949. https://doi.org/10.1093/mnras/sty2190 . arXiv:1801.05433 [astro-ph.SR]

Original

1949

Earlier work this paper cites.

Luyten WJ (1949) An Atlas of Identification Charts of White Dwarfs. ApJ 109:528. https://doi.org/10.1086/145156

1949

Earlier work this paper cites.

Spitzer J Lyman, Schwarzschild M (1951) The Possible Influence of Interstellar Clouds on Stellar Velocities. ApJ 114:385. https://doi.org/10.1086/145478

1951

Earlier work this paper cites.

Bondi H (1952) On spherically symmetrical accretion. MNRAS 112:195. https://doi.org/10.1093/mnras/112.2.195

1952

Earlier work this paper cites.

Haiman Z, Kocsis B, Menou K (2009) The Population of Viscosity- and Gravitational Wave-driven Supermassive Black Hole Binaries Among Luminous Active Galactic Nuclei. ApJ 700(2):1952–1969. https://doi.org/10.1088/0004-637X/700/2/1952 . arXiv:0904.1383 [astro-ph.CO]

Original

1952

Earlier work this paper cites.

Remmen GN, Wu K (2013) Complex orbital dynamics of a double neutron star system revolving around a massive black hole. MNRAS 430(3):1940–1955. https://doi.org/10.1093/mnras/stt023 . arXiv:1301.2836 [astro-ph.HE]

Original

1955

Earlier work this paper cites.

Blaauw A (1961) On the origin of the O- and B-type stars with high velocities (the “run-away” stars), and some related problems. Bull. Astron. Inst. Netherlands 15:265

1961

Earlier work this paper cites.

Bonnor WB, Rotenberg MA (1961) Transport of Momentum by Gravitational Waves: The Linear Approximation. Proceedings of the Royal Society of London Series A 265(1320):109–116. https://doi.org/10.1098/rspa.1961.0226

1961

Earlier work this paper cites.

Kozai Y (1962) Secular perturbations of asteroids with high inclination and eccentricity. AJ 67:591–598. https://doi.org/10.1086/108790

1962

Earlier work this paper cites.

Lidov ML (1962) The evolution of orbits of artificial satellites of planets under the action of gravitational perturbations of external bodies. Planet. Space Sci. 9(10):719–759. https://doi.org/10.1016/0032-0633(62)90129-0

1962

Earlier work this paper cites.

Peres A (1962) Classical Radiation Recoil. Physical Review 128(5):2471–2475. https://doi.org/10.1103/PhysRev.128.2471

1962

Earlier work this paper cites.

Peters PC, Mathews J (1963) Gravitational Radiation from Point Masses in a Keplerian Orbit. Physical Review 131(1):435–440. https://doi.org/10.1103/PhysRev.131.435

1963

Earlier work this paper cites.

Zahn JP (1966) Les marées dans une étoile double serrée. Annales d’Astrophysique 29:313

1966

Earlier work this paper cites.

Paczyński B (1967) Gravitational Waves and the Evolution of Close Binaries. Acta Astron. 17:287

1967

Earlier work this paper cites.

Carter B (1968) Global Structure of the Kerr Family of Gravitational Fields. Physical Review 174(5):1559–1571. https://doi.org/10.1103/PhysRev.174.1559

1968

Earlier work this paper cites.

Spitzer J Lyman (1969) Equipartition and the Formation of Compact Nuclei in Spherical Stellar Systems. ApJ 158:L139. https://doi.org/10.1086/180451

1969

Earlier work this paper cites.

Bardeen JM (1970) Kerr Metric Black Holes. Nature 226(5240):64–65. https://doi.org/10.1038/226064a0

1970

Earlier work this paper cites.

Gunn JE, Ostriker JP (1970) On the Nature of Pulsars. III. Analysis of Observations. ApJ 160:979. https://doi.org/10.1086/150487

1970

Earlier work this paper cites.

Faulkner J (1971) Ultrashort-Period Binaries, Gravitational Radiation, and Mass Transfer. I. The Standard Model, with Applications to WZ Sagittae and Z Camelopardalis. ApJ 170:L99. https://doi.org/10.1086/180848

1971

Earlier work this paper cites.

Vila SC (1971) Late Evolution of Close Binaries. ApJ 168:217. https://doi.org/10.1086/151076

1971

Earlier work this paper cites.

Hansen RO (1972) Post-Newtonian Gravitational Radiation from Point Masses in a Hyperbolic Kepler Orbit. Phys. Rev. D 5(4):1021–1023. https://doi.org/10.1103/PhysRevD.5.1021

1972

Earlier work this paper cites.

Paczyński B, Sienkiewicz R (1972) Evolution of Close Binaries VIII. Mass Exchange on the Dynamical Time Scale. Acta Astron. 22:73–91

1972

Earlier work this paper cites.

Bekenstein JD (1973) Gravitational-Radiation Recoil and Runaway Black Holes. ApJ 183:657–664. https://doi.org/10.1086/152255

1973

Earlier work this paper cites.

Novikov ID, Thorne KS (1973) Astrophysics of black holes. In: Black Holes (Les Astres Occlus). pp 343–450

1973

Earlier work this paper cites.

Shakura NI, Sunyaev RA (1973) Reprint of 1973A&A….24..337S. Black holes in binary systems. Observational appearance. A&A 500:33–51

1973

Earlier work this paper cites.

Trümper J, Schönfelder V (1973) Distance Determination of Variable X-ray Sources. A&A 25:445

1973

Earlier work this paper cites.

Press WH, Schechter P (1974) Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation. ApJ 187:425–438. https://doi.org/10.1086/152650

1974

Earlier work this paper cites.

Thorne KS (1974) Disk-Accretion onto a Black Hole. II. Evolution of the Hole. ApJ 191:507–520. https://doi.org/10.1086/152991

1974

Earlier work this paper cites.

Bardeen JM, Petterson JA (1975) The Lense-Thirring Effect and Accretion Disks around Kerr Black Holes. ApJ 195:L65. https://doi.org/10.1086/181711

1975

Earlier work this paper cites.

Fabian AC, Pringle JE, Rees MJ (1975) Tidal capture formation of binary systems and X-ray sources in globular clusters. MNRAS 172:15. https://doi.org/10.1093/mnras/172.1.15P

1975

Earlier work this paper cites.

Heggie DC (1975) Binary evolution in stellar dynamics. MNRAS 173:729–787. https://doi.org/10.1093/mnras/173.3.729

1975

Earlier work this paper cites.

Hulse RA, Taylor JH (1975) Discovery of a pulsar in a binary system. ApJ 195:L51–L53. https://doi.org/10.1086/181708

1975

Earlier work this paper cites.

Sutantyo W (1975) The formation of globular cluster X-ray sources through neutron star - giant collisions. A&A 44:227–230

1975

Earlier work this paper cites.

Tremaine SD, Ostriker JP, Spitzer J L (1975) The formation of the nuclei of galaxies. I. M31. ApJ 196:407–411. https://doi.org/10.1086/153422

1975

Earlier work this paper cites.

Bahcall JN, Wolf RA (1976) Star distribution around a massive black hole in a globular cluster. ApJ 209:214–232. https://doi.org/10.1086/154711

1976

Earlier work this paper cites.

Frank J, Rees MJ (1976) Effects of massive black holes on dense stellar systems. MNRAS 176:633–647. https://doi.org/10.1093/mnras/176.3.633

1976

Earlier work this paper cites.

Hills JG (1976) The formation of binaries containing black holes by the exchange of companions and the X-ray sources in globular clusters. MNRAS 175:1P–4P. https://doi.org/10.1093/mnras/175.1.1P

1976

Earlier work this paper cites.

Paczynski B (1976) Common Envelope Binaries. In: Eggleton P, Mitton S, Whelan J (eds) Structure and Evolution of Close Binary Systems. IAUS, vol 73. p 75

1976

Earlier work this paper cites.

Shakura NI, Sunyaev RA (1976) A theory of the instability of disk accretion on to black holes and the variability of binary X-ray sources, galactic nuclei and quasars. MNRAS 175:613–632. https://doi.org/10.1093/mnras/175.3.613

1976

Earlier work this paper cites.

Smarr LL, Blandford R (1976) The binary pulsar: physical processes, possible companions, and evolutionary histories. ApJ 207:574–588. https://doi.org/10.1086/154524

1976

Earlier work this paper cites.

Tremaine SD (1976) The formation of the nuclei of galaxies. II. The local group. ApJ 203:345–351. https://doi.org/10.1086/154085

1976

Earlier work this paper cites.

van den Heuvel EPJ (1976) Late Stages of Close Binary Systems. In: Eggleton P, Mitton S, Whelan J (eds) Structure and Evolution of Close Binary Systems. IAU Symposium, vol 73. p 35

1976

Earlier work this paper cites.

Blandford RD, Znajek RL (1977) Electromagnetic extraction of energy from Kerr black holes. MNRAS 179:433–456. https://doi.org/10.1093/mnras/179.3.433

1977

Earlier work this paper cites.

Komossa S (2012) Recoiling Black Holes: Electromagnetic Signatures, Candidates, and Astrophysical Implications. Advances in Astronomy 2012:364973. https://doi.org/10.1155/2012/364973 . arXiv:1202.1977 [astro-ph.CO]

Original

1977

Earlier work this paper cites.

Zahn JP (1977) Reprint of 1977A&A….57..383Z. Tidal friction in close binary stars. A&A 500:121–132

1977

Earlier work this paper cites.

Arnold VI (1978) Mathematical methods of classical mechanics. Springer - Verlag

1978

Earlier work this paper cites.

Cohn H, Kulsrud RM (1978) The stellar distribution around a black hole: numerical integration of the Fokker-Planck equation. ApJ 226:1087–1108. https://doi.org/10.1086/156685

1978

Earlier work this paper cites.

Shapiro SL, Marchant AB (1978) Star clusters containing massive, central black holes: Monte Carlo simulations in two-dimensional phase space. ApJ 225:603–624. https://doi.org/10.1086/156521

1978

Earlier work this paper cites.

Mazeh T, Shaham J (1979) The orbital evolution of close triple systems: the binary eccentricity. A&A 77:145

1979

Earlier work this paper cites.

Webbink RF (1979) The evolution of low-mass close binary systems. VI. Population II W Ursae Majoris systems. ApJ 227:178–184. https://doi.org/10.1086/156717

1979

Earlier work this paper cites.

Begelman MC, Blandford RD, Rees MJ (1980) Massive black hole binaries in active galactic nuclei. Nature 287(5780):307–309. https://doi.org/10.1038/287307a0

1980

Earlier work this paper cites.

Connors PA, Piran T, Stark RF (1980) Polarization features of X-ray radiation emitted near black holes. ApJ 235:224–244. https://doi.org/10.1086/157627

1980

Earlier work this paper cites.

Hills JG, Fullerton LW (1980) Computer simulations of close encounters between single stars and hard binaries. AJ 85:1281–1291. https://doi.org/10.1086/112798

1980

Earlier work this paper cites.

Hut P (1981) Tidal evolution in close binary systems. A&A 99:126–140

1981

Earlier work this paper cites.

Rappaport S, Joss PC, Webbink RF (1982) The evolution of highly compact binary stellar systems. ApJ 254:616–640. https://doi.org/10.1086/159772

1982

Earlier work this paper cites.

Soltan A (1982) Masses of quasars. MNRAS 200:115–122. https://doi.org/10.1093/mnras/200.1.115

1982

Earlier work this paper cites.

Carter B, Luminet JP (1983) Tidal compression of a star by a large black hole. I Mechanical evolution and nuclear energy release by proton capture. A&A 121(1):97–113

1983

Earlier work this paper cites.

Eggleton PP (1983) Aproximations to the radii of Roche lobes. ApJ 268:368–369. https://doi.org/10.1086/160960

1983

Earlier work this paper cites.

Fitchett MJ (1983) The influence of gravitational wave momentum losses on the centre of mass motion of a Newtonian binay system. MNRAS 203:1049–1062. https://doi.org/10.1093/mnras/203.4.1049

1983

Earlier work this paper cites.

Hellings RW, Downs GS (1983) Upper limits on the isotopic gravitational radiation background frompulsar timing analysis. ApJ 265:L39–L42. https://doi.org/10.1086/183954

1983

Earlier work this paper cites.

Hut P, Bahcall JN (1983) Binary-single star scattering. I - Numerical experiments for equal masses. ApJ 268:319–341. https://doi.org/10.1086/160956

1983

Earlier work this paper cites.

Mikkola S (1983) Encounters of binaries. I - Equal energies. MNRAS 203:1107–1121. https://doi.org/10.1093/mnras/203.4.1107

1983

Earlier work this paper cites.

Hut P, Paczynski B (1984) Effects of encoounters with field stars on the evolution of low-mass semidetached binaries. ApJ 284:675–684. https://doi.org/10.1086/162450

1984

Earlier work this paper cites.

Livio M, Soker N (1984) Star-planet systems as possible progenitors of cataclysmic binaries. MNRAS 208:763–781. https://doi.org/10.1093/mnras/208.4.763

1984

Earlier work this paper cites.

Mikkola S (1984) Encounters of binaries. II - Unequal energies. MNRAS 207:115–126. https://doi.org/10.1093/mnras/207.1.115

1984

Earlier work this paper cites.

Tremaine S, Weinberg MD (1984) Dynamical friction in spherical systems. MNRAS 209:729–757. https://doi.org/10.1093/mnras/209.4.729

1984

Earlier work this paper cites.

Webbink RF (1984) Double white dwarfs as progenitors of R Coronae Borealis stars and type I supernovae. ApJ 277:355–360. https://doi.org/10.1086/161701

1984

Earlier work this paper cites.

Zinn R, West MJ (1984) The globular cluster system of the Galaxy. III. Measurements of radial velocity and metallicity for 60 clusters and a compilation of metallicities for 121 clusters. ApJS 55:45–66. https://doi.org/10.1086/190947

1984

Earlier work this paper cites.

Ma L, Hopkins PF, Ma X, Anglés-Alcázar D, Faucher-Giguère CA, Kelley LZ (2021) Seeds don’t sink: even massive black hole ’seeds’ cannot migrate to galaxy centres efficiently. MNRAS 508(2):1973–1985. https://doi.org/10.1093/mnras/stab2713 . arXiv:2101.02727 [astro-ph.GA]

Original

1985

Earlier work this paper cites.

Webbink RF (1985) Stellar evolution and binaries, p 39

1985

Earlier work this paper cites.

Byrd GG, Valtonen MJ, Sundelius B, Valtaoja L (1986) Tidal triggering of Seyfert galaxies and quasars : perturbed galaxy disk models versus observations. A&A 166:75–82

1986

Earlier work this paper cites.

Habets GMHJ (1986) The evolution of a single and a binary helium star of 2.5 solar mass up to neon ignition. A&A 165:95–109

1986

Earlier work this paper cites.

Nelson LA, Rappaport SA, Joss PC (1986) The Evolution of Ultrashort Period Binary Systems. ApJ 304:231. https://doi.org/10.1086/164156

1986

Earlier work this paper cites.

Paczynski B (1986) Gamma-ray bursters at cosmological distances. ApJ 308:L43–L46. https://doi.org/10.1086/184740

1986

Earlier work this paper cites.

Weinberg MD (1986) Orbital Decay of Satellite Galaxies in Spherical Systems. ApJ 300:93. https://doi.org/10.1086/163785

1986

Earlier work this paper cites.

Binney J, Tremaine S (1987) Galactic dynamics. Princeton Univeristy Press

1987

Earlier work this paper cites.

Hjellming MS, Webbink RF (1987) Thresholds for Rapid Mass Transfer in Binary System. I. Polytropic Models. ApJ 318:794. https://doi.org/10.1086/165412

1987

Earlier work this paper cites.

Spitzer L (1987) Dynamical evolution of globular clusters

1987

Earlier work this paper cites.

Stella L (1987) A 685 second orbital period from the X-ray source 4U 1820-30 in the globular cluster NGC 6624. In: Variability of Galactic and Extragalactic X-ray Sources. pp 157–164

1987

Earlier work this paper cites.

Stella L, Priedhorsky W, White NE (1987) The Discovery of a Second Orbital Period from the X-Ray Source 4U 1820-30 in the Globular Cluster NGC 6624. ApJ 312:L17. https://doi.org/10.1086/184811

1987

Earlier work this paper cites.

Bahcall NA (1988) Large-scale structure in the universe indicated by galaxy clusters. ARA&A 26:631–686. https://doi.org/10.1146/annurev.aa.26.090188.003215

1988

Earlier work this paper cites.

Fruchter AS, Stinebring DR, Taylor JH (1988) A millisecond pulsar in an eclipsing binary. Nature 333(6170):237–239. https://doi.org/10.1038/333237a0

1988

Earlier work this paper cites.

Rees MJ (1988) Tidal disruption of stars by black holes of 10 6

1988

Earlier work this paper cites.

Ward WR (1988) On disk-planet interactions and orbital eccentricities. Icarus 73(2):330–348. https://doi.org/10.1016/0019-1035(88)90103-0

1988

Earlier work this paper cites.

Webbink RF, Iben IJ (1988) 2d Conf.on Faint Blue Stars, Schenectady: L. Davis Press. p 445

1988

Earlier work this paper cites.

Phinney ES (1989) Manifestations of a Massive Black Hole in the Galactic Center. In: Morris M (ed) The Center of the Galaxy. IAU Symposium, vol 136. p 543

1989

Earlier work this paper cites.

Quinlan GD, Shapiro SL (1989) Dynamical Evolution of Dense Clusters of Compact Stars. ApJ 343:725. https://doi.org/10.1086/167745

1989

Earlier work this paper cites.

Redmount IH, Rees MJ (1989) Gravitational-radiation rocket effects and galactic structure. Comments on Astrophysics 14:165

1989

Earlier work this paper cites.

Shlosman I, Begelman MC (1989) Evolution of Self-Gravitating Accretion Disks in Active Galactic Nuclei. ApJ 341:685. https://doi.org/10.1086/167526

1989

Earlier work this paper cites.

Weinberg MD (1989) Self-gravitating response of a spherical galaxy to sinking satellites. MNRAS 239:549–569. https://doi.org/10.1093/mnras/239.2.549

1989

Earlier work this paper cites.

Hils D, Bender PL, Webbink RF (1990) Gravitational Radiation from the Galaxy. ApJ 360:75. https://doi.org/10.1086/169098

1990

Earlier work this paper cites.

King AR, Frank J, Whitehurst R (1990) Synchronous rotation in AM Herculis systems-I. Equilibrium configurations. MNRAS 244:731

1990

Earlier work this paper cites.

Kochanek CS, Shapiro SL, Teukolsky SA, Chernoff DF (1990) Gravitational Radiation from Colliding Clusters: Newtonian Simulations in Three Dimensions. ApJ 358:81. https://doi.org/10.1086/168964

1990

Earlier work this paper cites.

Mikkola S, Valtonen MJ (1990) The Slingshot Ejections in Merging Galaxies. ApJ 348:412. https://doi.org/10.1086/168250

1990

Earlier work this paper cites.

Bhattacharya D, van den Heuvel EPJ (1991) Formation and evolution of binary and millisecond radio pulsars. Phys. Rep. 203(1-2):1–124. https://doi.org/10.1016/0370-1573(91)90064-S

1991

Earlier work this paper cites.

Ebisuzaki T, Makino J, Okumura SK (1991) Merging of two galaxies with central black holes. Nature 354(6350):212–214. https://doi.org/10.1038/354212a0

1991

Earlier work this paper cites.

McMillan S, Hut P, Makino J (1991) Star Cluster Evolution with Primordial Binaries. II. Detailed Analysis. ApJ 372:111. https://doi.org/10.1086/169958

1991

Earlier work this paper cites.

Phinney ES (1991) The Rate of Neutron Star Binary Mergers in the Universe: Minimal Predictions for Gravity Wave Detectors. ApJ 380:L17. https://doi.org/10.1086/186163

1991

Earlier work this paper cites.

Podsiadlowski P (1991) Irradiation-driven mass transfer in low-mass X-ray binaries. Nature 350(6314):136–138. https://doi.org/10.1038/350136a0

1991

Earlier work this paper cites.

Syer D, Clarke CJ, Rees MJ (1991) Star-disc interactions near a massive black hole. MNRAS 250:505–512. https://doi.org/10.1093/mnras/250.3.505

1991

Earlier work this paper cites.

Tan J, Morgan E, Lewin WHG, Penninx W, van der Klis M, van Paradijs J, Makishima K, Inoue H, Dotani T, Mitsuda K (1991) Changes in the 11 Minute Period of 4U 1820-30. ApJ 374:291. https://doi.org/10.1086/170118

1991

Earlier work this paper cites.

Bildsten L, Cutler C (1992) Tidal Interactions of Inspiraling Compact Binaries. ApJ 400:175. https://doi.org/10.1086/171983

1992

Earlier work this paper cites.

Bildsten L, Salpeter EE, Wasserman I (1992) The Fate of Accreted CNO Elements in Neutron Star Atmospheres: X-Ray Bursts and Gamma-Ray Lines. ApJ 384:143. https://doi.org/10.1086/170860

1992

Earlier work this paper cites.

Halpern JP, Holt SS (1992) Discovery of soft X-ray pulsations from the γ \gamma -ray source Geminga. Nature 357(6375):222–224. https://doi.org/10.1038/357222a0

1992

Earlier work this paper cites.

Hut P, McMillan S, Goodman J, Mateo M, Phinney ES, Pryor C, Richer HB, Verbunt F, Weinberg M (1992) Binaries in Globular Clusters. PASP 104:981. https://doi.org/10.1086/133085

1992

Earlier work this paper cites.

Kochanek CS (1992) Coalescing Binary Neutron Stars. ApJ 398:234. https://doi.org/10.1086/171851

1992

Earlier work this paper cites.

Mikkola S, Valtonen MJ (1992) Evolution of binaries in the field of light particles and the problem of two black holes. MNRAS 259(1):115–120. https://doi.org/10.1093/mnras/259.1.115

1992

Earlier work this paper cites.

Narayan R, Paczynski B, Piran T (1992) Gamma-Ray Bursts as the Death Throes of Massive Binary Stars. ApJ 395:L83. https://doi.org/10.1086/186493 . arXiv:astro-ph/9204001 [astro-ph]

1992

Earlier work this paper cites.

Tavani M, Brookshaw L (1992) The origin of planets orbiting millisecond pulsars. Nature 356(6367):320–322. https://doi.org/10.1038/356320a0

1992

Earlier work this paper cites.

Artymowicz P, Lin DNC, Wampler EJ (1993) Star Trapping and Metallicity Enrichment in Quasars and Active Galactic Nuclei. ApJ 409:592. https://doi.org/10.1086/172690

1993

Earlier work this paper cites.

Capuzzo-Dolcetta R (1993) The Evolution of the Globular Cluster System in a Triaxial Galaxy: Can a Galactic Nucleus Form by Globular Cluster Capture? ApJ 415:616. https://doi.org/10.1086/173189 . arXiv:astro-ph/9301006 [astro-ph]

1993

Earlier work this paper cites.

Goodman J, Hut P (1993) Binary–Single-Star Scattering. V. Steady State Binary Distribution in a Homogeneous Static Background of Single Stars. ApJ 403:271. https://doi.org/10.1086/172200

1993

Earlier work this paper cites.

Kauffmann G, White SDM, Guiderdoni B (1993) The formation and evolution of galaxies within merging dark matter haloes. MNRAS 264:201–218. https://doi.org/10.1093/mnras/264.1.201

1993

Earlier work this paper cites.

Kolb U (1993) A model for the intrinsic population of cataclysmic variables. A&A 271:149

1993

Earlier work this paper cites.

Lacey C, Cole S (1993) Merger rates in hierarchical models of galaxy formation. MNRAS 262(3):627–649. https://doi.org/10.1093/mnras/262.3.627

1993

Earlier work this paper cites.

Morris M (1993) Massive Star Formation near the Galactic Center and the Fate of the Stellar Remnants. ApJ 408:496. https://doi.org/10.1086/172607

1993

Earlier work this paper cites.

Sigurdsson S, Phinney ES (1993) Binary–Single Star Interactions in Globular Clusters. ApJ 415:631. https://doi.org/10.1086/173190

1993

Earlier work this paper cites.

Tutukov AV, Yungelson LR (1993) The merger rate of neutron star and black hole binaries. MNRAS 260:675–678. https://doi.org/10.1093/mnras/260.3.675

1993

Earlier work this paper cites.

Woosley SE (1993) Gamma-Ray Bursts from Stellar Mass Accretion Disks around Black Holes. ApJ 405:273. https://doi.org/10.1086/172359

1993

Earlier work this paper cites.

Apostolatos TA, Cutler C, Sussman GJ, Thorne KS (1994) Spin-induced orbital precession and its modulation of the gravitational waveforms from merging binaries. Phys. Rev. D 49(12):6274–6297. https://doi.org/10.1103/PhysRevD.49.6274

1994

Earlier work this paper cites.

Applegate JH, Shaham J (1994) Orbital Period Variability in the Eclipsing Pulsar Binary PSR B1957+20: Evidence for a Tidally Powered Star. ApJ 436:312. https://doi.org/10.1086/174906

1994

Earlier work this paper cites.

Cutler C, Flanagan ÉE (1994) Gravitational waves from merging compact binaries: How accurately can one extract the binary’s parameters from the inspiral waveform? Phys. Rev. D 49(6):2658–2697. https://doi.org/10.1103/PhysRevD.49.2658 . arXiv:gr-qc/9402014 [gr-qc]

1994

Earlier work this paper cites.

Haehnelt MG (1994) Low-Frequency Gravitational Waves from Supermassive Black-Holes. MNRAS 269:199. https://doi.org/10.1093/mnras/269.1.199 . arXiv:astro-ph/9405032 [astro-ph]

1994

Earlier work this paper cites.

Kiseleva LG, Eggleton PP, Orlov VV (1994) Instability of close triple systems with coplanar initial doubly circular motion. MNRAS 270:936–946. https://doi.org/10.1093/mnras/270.4.936

1994

Earlier work this paper cites.

Lai D, Rasio FA, Shapiro SL (1994) Hydrodynamics of Rotating Stars and Close Binary Interactions: Compressible Ellipsoid Models. ApJ 437:742. https://doi.org/10.1086/175036 . arXiv:astro-ph/9404031 [astro-ph]

1994

Earlier work this paper cites.

Moore B (1994) Evidence against dissipation-less dark matter from observations of galaxy haloes. Nature 370(6491):629–631. https://doi.org/10.1038/370629a0

1994

Earlier work this paper cites.

Narayan R, Yi I (1994) Advection-dominated Accretion: A Self-similar Solution. ApJ 428:L13. https://doi.org/10.1086/187381 . arXiv:astro-ph/9403052 [astro-ph]

1994

Earlier work this paper cites.

Poveda A, Herrera MA, Allen C, Cordero G, Lavalley C (1994) Statistical studies of visual double and multiple stars. II. A catalogue of nearby wide binary and multiple systems. Rev. Mexicana Astron. Astrofis. 28:43–89

1994

Earlier work this paper cites.

Ravenhall DG, Pethick CJ (1994) Neutron Star Moments of Inertia. ApJ 424:846. https://doi.org/10.1086/173935

1994

Earlier work this paper cites.

Shore SN, Livio M, van den Heuvel EPJ (1994) Interacting binaries

1994

Earlier work this paper cites.

Grindlay JE, Cool AM, Callanan PJ, Bailyn CD, Cohn HN, Lugger PM (1995) Spectroscopic Identification of Probable Cataclysmic Variables in the Globular Cluster NGC 6397. ApJ 455:L47. https://doi.org/10.1086/309806

1995

Earlier work this paper cites.

Kidder LE (1995) Coalescing binary systems of compact objects to (post) 5/2

1995

Earlier work this paper cites.

Kormendy J, Richstone D (1995) Inward Bound—The Search For Supermassive Black Holes In Galactic Nuclei. ARA&A 33:581. https://doi.org/10.1146/annurev.aa.33.090195.003053

1995

Earlier work this paper cites.

Lai D, Shapiro SL (1995) Hydrodynamics of Coalescing Binary Neutron Stars: Ellipsoidal Treatment. ApJ 443:705. https://doi.org/10.1086/175562 . arXiv:astro-ph/9408054 [astro-ph]

1995

Earlier work this paper cites.

Lee HM (1995) Evolution of galactic nuclei with 10-M_ black holes. MNRAS 272(3):605–617. https://doi.org/10.1093/mnras/272.3.605 . arXiv:astro-ph/9409073 [astro-ph]

1995

Earlier work this paper cites.

Marsh TR, Dhillon VS, Duck SR (1995) Low-Mass White Dwarfs Need Friends - Five New Double-Degenerate Close Binary Stars. MNRAS 275:828. https://doi.org/10.1093/mnras/275.3.828

1995

Earlier work this paper cites.

Poisson E, Will CM (1995) Gravitational waves from inspiraling compact binaries: Parameter estimation using second-post-Newtonian waveforms. Phys. Rev. D 52:848–855. arXiv:gr-qc/9502040

1995

Earlier work this paper cites.

Warner B (1995) The AM Canum Venaticorum Stars. Ap&SS 225(2):249–270. https://doi.org/10.1007/BF00613240

1995

Earlier work this paper cites.

Bade N, Komossa S, Dahlem M (1996) Detection of an extremely soft X-ray outburst in the HII-like nucleus of NGC 5905. A&A 309:L35–L38

1996

Earlier work this paper cites.

Carlberg RG, Yee HKC, Ellingson E, Abraham R, Gravel P, Morris S, Pritchet CJ (1996) Galaxy Cluster Virial Masses and Omega. ApJ 462:32. https://doi.org/10.1086/177125 . arXiv:astro-ph/9509034 [astro-ph]

1996

Earlier work this paper cites.

Girardi M, Fadda D, Giuricin G, Mardirossian F, Mezzetti M, Biviano A (1996) Velocity Dispersions and X-Ray Temperatures of Galaxy Clusters. ApJ 457:61. https://doi.org/10.1086/176711 . arXiv:astro-ph/9507031 [astro-ph]

1996

Earlier work this paper cites.

Lipunov VM, Postnov KA, Prokhorov ME (1996) The scenario machine: Binary star population synthesis

1996

Earlier work this paper cites.

Owen BJ (1996) Search templates for gravitational waves from inspiraling binaries: Choice of template spacing. Phys. Rev. D 53(12):6749–6761. https://doi.org/10.1103/PhysRevD.53.6749 . arXiv:gr-qc/9511032 [gr-qc]

1996

Earlier work this paper cites.

Portegies Zwart SF, Verbunt F (1996) Population synthesis of high-mass binaries. A&A 309:179–196

1996

Earlier work this paper cites.

Quinlan GD (1996) The dynamical evolution of massive black hole binaries I. Hardening in a fixed stellar background. New A 1(1):35–56. https://doi.org/10.1016/S1384-1076(96)00003-6 . arXiv:astro-ph/9601092 [astro-ph]

1996

Earlier work this paper cites.

Rasio FA, Livio M (1996) On the Formation and Evolution of Common Envelope Systems. ApJ 471:366. https://doi.org/10.1086/177975 . arXiv:astro-ph/9511054 [astro-ph]

1996

Earlier work this paper cites.

Rauch KP, Tremaine S (1996) Resonant relaxation in stellar systems. New A 1(2):149–170. https://doi.org/10.1016/S1384-1076(96)00012-7 . arXiv:astro-ph/9603018 [astro-ph]

1996

Earlier work this paper cites.

Ward WR (1997) Protoplanet Migration by Nebula Tides. Icarus 126(2):261–281. https://doi.org/10.1006/icar.1996.5647

1996

Earlier work this paper cites.

Bender PL, Hils D (1997) Confusion noise level due to galactic and extragalactic binaries. Classical and Quantum Gravity 14(6):1439–1444. https://doi.org/10.1088/0264-9381/14/6/008

1997

Earlier work this paper cites.

Kahabka P, van den Heuvel EPJ (1997) Luminous Supersoft X-Ray Sources. ARA&A 35:69–100. https://doi.org/10.1146/annurev.astro.35.1.69

1997

Earlier work this paper cites.

Nandra K, George IM, Mushotzky RF, Turner TJ, Yaqoob T (1997) ASCA Observations of Seyfert 1 Galaxies. II. Relativistic Iron K α \alpha Emission. ApJ 477(2):602–622. https://doi.org/10.1086/303721 . arXiv:astro-ph/9606169 [astro-ph]

1997

Earlier work this paper cites.

Provencal JL, Winget DE, Nather RE, Robinson EL, Clemens JC, Bradley PA, Claver CF, Kleinman SJ, Grauer AD, Hine BP, et al. (1997) Whole Earth Telescope Observations of the Helium Interacting Binary PG 1346+082 (CR Bootis). ApJ 480(1):383–394. https://doi.org/10.1086/303971

1997

Earlier work this paper cites.

Quinlan GD, Hernquist L (1997) The dynamical evolution of massive black hole binaries — II. Self-consistent N-body integrations. New A 2(6):533–554. https://doi.org/10.1016/S1384-1076(97)00039-0 . arXiv:astro-ph/9706298 [astro-ph]

1997

Earlier work this paper cites.

Sigurdsson S, Rees MJ (1997) Capture of stellar mass compact objects by massive black holes in galactic cusps. MNRAS 284(2):318–326. https://doi.org/10.1093/mnras/284.2.318 . arXiv:astro-ph/9608093 [astro-ph]

1997

Earlier work this paper cites.

Soberman GE, Phinney ES, van den Heuvel EPJ (1997) Stability criteria for mass transfer in binary stellar evolution. A&A 327:620–635. arXiv:astro-ph/9703016 [astro-ph]

1997

Earlier work this paper cites.

Duncan MJ, Lissauer JJ (1998) The Effects of Post-Main-Sequence Solar Mass Loss on the Stability of Our Planetary System. Icarus 134(2):303–310. https://doi.org/10.1006/icar.1998.5962

1998

Earlier work this paper cites.

Haehnelt MG, Natarajan P, Rees MJ (1998) High-redshift galaxies, their active nuclei and central black holes. MNRAS 300(3):817–827. https://doi.org/10.1046/j.1365-8711.1998.01951.x . arXiv:astro-ph/9712259 [astro-ph]

1998

Earlier work this paper cites.

Iben J Icko, Tutukov AV, Fedorova ArV (1998) On the Luminosity of White Dwarfs in Close Binaries Merging under the Influence of Gravitational Wave Radiation. ApJ 503(1):344–349. https://doi.org/10.1086/305972

1998

Earlier work this paper cites.

Kiseleva LG, Eggleton PP, Mikkola S (1998) Tidal friction in triple stars. MNRAS 300(1):292–302. https://doi.org/10.1046/j.1365-8711.1998.01903.x

1998

Earlier work this paper cites.

Magorrian J, Tremaine S, Richstone D, Bender R, Bower G, Dressler A, Faber SM, Gebhardt K, Green R, Grillmair C, et al. (1998) The Demography of Massive Dark Objects in Galaxy Centers. AJ 115(6):2285–2305. https://doi.org/10.1086/300353 . arXiv:astro-ph/9708072 [astro-ph]

1998

Earlier work this paper cites.

Nelemans G, Tauris TM (1998) Formation of undermassive single white dwarfs and the influence of planets on late stellar evolution. A&A 335:L85–L88. arXiv:astro-ph/9806011 [astro-ph]

1998

Earlier work this paper cites.

Popham R, Gammie CF (1998) Advection-dominated Accretion Flows in the Kerr Metric. II. Steady State Global Solutions. ApJ 504(1):419–430. https://doi.org/10.1086/306054 . arXiv:astro-ph/9802321 [astro-ph]

1998

Earlier work this paper cites.

Portegies Zwart SF, Yungelson LR (1998) Formation and evolution of binary neutron stars. A&A 332:173–188. arXiv:astro-ph/9710347 [astro-ph]

1998

Earlier work this paper cites.

Saffer RA, Livio M, Yungelson LR (1998) Close Binary White Dwarf Systems: Numerous New Detections and Their Interpretation. ApJ 502(1):394–407. https://doi.org/10.1086/305907 . arXiv:astro-ph/9802356 [astro-ph]

1998

Earlier work this paper cites.

Bloom JS, Sigurdsson S, Pols OR (1999) The spatial distribution of coalescing neutron star binaries: implications for gamma-ray bursts. MNRAS 305(4):763–769. https://doi.org/10.1046/j.1365-8711.1999.02437.x . arXiv:astro-ph/9805222 [astro-ph]

1999

Earlier work this paper cites.

Buonanno A, Damour T (1999) Effective one-body approach to general relativistic two-body dynamics. Phys. Rev. D 59(8):084006. https://doi.org/10.1103/PhysRevD.59.084006 . arXiv:gr-qc/9811091 [gr-qc]

1999

Earlier work this paper cites.

Gondolo P, Silk J (1999) Dark Matter Annihilation at the Galactic Center. Phys. Rev. Lett. 83(9):1719–1722. https://doi.org/10.1103/PhysRevLett.83.1719 . arXiv:astro-ph/9906391 [astro-ph]

1999

Earlier work this paper cites.

Grupe D, Thomas HC, Leighly KM (1999) RX J1624.9+7554: a new X-ray transient AGN. A&A 350:L31–L34. arXiv:astro-ph/9909101 [astro-ph]

1999

Earlier work this paper cites.

Hachisu I, Kato M, Nomoto K (1999) A Wide Symbiotic Channel to Type IA Supernovae. ApJ 522(1):487–503. https://doi.org/10.1086/307608 . arXiv:astro-ph/9902304 [astro-ph]

1999

Earlier work this paper cites.

Kato M, Hachisu I (1999) A New Estimation of Mass Accumulation Efficiency in Helium Shell Flashestoward Type IA Supernova Explosions. ApJ 513(1):L41–L44. https://doi.org/10.1086/311893 . arXiv:astro-ph/9901080 [astro-ph]

1999

Earlier work this paper cites.

Komossa S, Greiner J (1999) Discovery of a giant and luminous X-ray outburst from the optically inactive galaxy pair RX J1242.6-1119. A&A 349:L45–L48. arXiv:astro-ph/9908216 [astro-ph]

1999

Earlier work this paper cites.

Mardling R, Aarseth S (1999) Dynamics and Stability of Three-Body Systems. In: Steves BA, Roy AE (eds) The Dynamics of Small Bodies in the Solar System, A Major Key to Solar System Studies. NATO Advanced Study Institute (ASI) Series C, vol 522. p 385

1999

Earlier work this paper cites.

Murray CD, Dermott SF (1999) Solar system dynamics

1999

Earlier work this paper cites.

Ostriker EC (1999) Dynamical Friction in a Gaseous Medium. ApJ 513(1):252–258. https://doi.org/10.1086/306858 . arXiv:astro-ph/9810324 [astro-ph]

1999

Earlier work this paper cites.

Skillman DR, Patterson J, Kemp J, Harvey DA, Fried RE, Retter A, Lipkin Y, Vanmunster T (1999) Superhumps in Cataclysmic Binaries. XVII. AM Canum Venaticorum. PASP 111(764):1281–1291. https://doi.org/10.1086/316437

1999

Earlier work this paper cites.

Tauris TM, Savonije GJ (1999) Formation of millisecond pulsars. I. Evolution of low-mass X-ray binaries with P_orb> 2 days. A&A 350:928–944. arXiv:astro-ph/9909147 [astro-ph]

1999

Earlier work this paper cites.

Thorsett SE, Arzoumanian Z, Camilo F, Lyne AG (1999) The Triple Pulsar System PSR B1620-26 in M4. ApJ 523(2):763–770. https://doi.org/10.1086/307771 . arXiv:astro-ph/9903227 [astro-ph]

1999

Earlier work this paper cites.

Ulmer A (1999) Flares from the Tidal Disruption of Stars by Massive Black Holes. ApJ 514(1):180–187. https://doi.org/10.1086/306909

1999

Earlier work this paper cites.

Binggeli B, Barazza F, Jerjen H (2000) Off-center nuclei in dwarf elliptical galaxies. A&A 359:447–456

2000

Earlier work this paper cites.

Buonanno A, Damour T (2000) Transition from inspiral to plunge in binary black hole coalescences. Phys. Rev. D 62(6):064015. https://doi.org/10.1103/PhysRevD.62.064015 . arXiv:gr-qc/0001013 [gr-qc]

2000

Earlier work this paper cites.

Fabian AC, Iwasawa K, Reynolds CS, Young AJ (2000) Broad Iron Lines in Active Galactic Nuclei. PASP 112(775):1145–1161. https://doi.org/10.1086/316610 . arXiv:astro-ph/0004366 [astro-ph]

2000

Earlier work this paper cites.

Ferrarese L, Merritt D (2000) A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies. ApJ 539(1):L9–L12. https://doi.org/10.1086/312838 . arXiv:astro-ph/0006053 [astro-ph]

2000

Earlier work this paper cites.

Ford EB, Kozinsky B, Rasio FA (2000) Secular Evolution of Hierarchical Triple Star Systems. ApJ 535(1):385–401. https://doi.org/10.1086/308815

2000

Earlier work this paper cites.

Gebhardt K, Bender R, Bower G, Dressler A, Faber SM, Filippenko AV, Green R, Grillmair C, Ho LC, Kormendy J, et al. (2000) A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion. ApJ 539(1):L13–L16. https://doi.org/10.1086/312840 . arXiv:astro-ph/0006289 [astro-ph]

2000

Earlier work this paper cites.

Greiner J, Schwarz R, Zharikov S, Orio M (2000) RX J1420.4+5334 - another tidal disruption event? A&A 362:L25–L28. arXiv:astro-ph/0009430 [astro-ph]

2000

Earlier work this paper cites.

Kauffmann G, Haehnelt M (2000) A unified model for the evolution of galaxies and quasars. MNRAS 311(3):576–588. https://doi.org/10.1046/j.1365-8711.2000.03077.x . arXiv:astro-ph/9906493 [astro-ph]

2000

Earlier work this paper cites.

Maggiore M (2000) Stochastic backgrounds of gravitational waves. arXiv e-prints gr-qc/0008027. arXiv:gr-qc/0008027 [astro-ph]

2000

Earlier work this paper cites.

Maxted PFL, Marsh TR, Moran CKJ (2000a) Radial velocity measurements of white dwarfs. MNRAS 319(1):305–317. https://doi.org/10.1046/j.1365-8711.2000.03840.x . arXiv:astro-ph/0007129 [astro-ph]

2000

Earlier work this paper cites.

Maxted PFL, Marsh TR, Moran CKJ, Han Z (2000b) The triple degenerate star WD 1704+481. MNRAS 314(2):334–337. https://doi.org/10.1046/j.1365-8711.2000.03343.x . arXiv:astro-ph/0001212 [astro-ph]

2000

Earlier work this paper cites.

Nelemans G, Verbunt F, Yungelson LR, Portegies Zwart SF (2000) Reconstructing the evolution of double helium white dwarfs: envelope loss without spiral-in. A&A 360:1011–1018. arXiv:astro-ph/0006216 [astro-ph]

2000

Earlier work this paper cites.

Portegies Zwart SF, McMillan SLW (2000) Black Hole Mergers in the Universe. ApJ 528(1):L17–L20. https://doi.org/10.1086/312422 . arXiv:astro-ph/9910061 [astro-ph]

2000

Earlier work this paper cites.

Sandquist EL, Taam RE, Burkert A (2000) On the Formation of Helium Double Degenerate Stars and Pre-Cataclysmic Variables. ApJ 533(2):984–997. https://doi.org/10.1086/308687 . arXiv:astro-ph/9912243 [astro-ph]

2000

Earlier work this paper cites.

Tauris TM, Sennels T (2000) Formation of the binary pulsars PSR B2303+46 and PSR J1141-6545. Young neutron stars with old white dwarf companions. A&A 355:236–244. arXiv:astro-ph/9909149 [astro-ph]

2000

Earlier work this paper cites.

Tauris TM, van den Heuvel EPJ, Savonije GJ (2000) Formation of Millisecond Pulsars with Heavy White Dwarf Companions:Extreme Mass Transfer on Subthermal Timescales. ApJ 530(2):L93–L96. https://doi.org/10.1086/312496 . arXiv:astro-ph/0001013 [astro-ph]

2000

Earlier work this paper cites.

Abbott BP, Abbott R, Abbott TD, Abraham S, Acernese F, Ackley K, Adams C, Adhikari RX, Adya VB, Affeldt C, et al. (2020a) GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ \sim 3.4 M ⊙

Original

2001

Earlier work this paper cites.

Barausse E, Berti E, Hertog T, Hughes SA, Jetzer P, Pani P, Sotiriou TP, Tamanini N, Witek H, Yagi K, et al. (2020a) Prospects for fundamental physics with LISA. General Relativity and Gravitation 52(8):81. https://doi.org/10.1007/s10714-020-02691-1 . arXiv:2001.09793 [gr-qc]

Original

2001

Earlier work this paper cites.

Bonetti M, Rasskazov A, Sesana A, Dotti M, Haardt F, Leigh NWC, Arca Sedda M, Fragione G, Rossi E (2020b) On the eccentricity evolution of massive black hole binaries in stellar backgrounds. MNRAS 493(1):L114–L119. https://doi.org/10.1093/mnrasl/slaa018 . arXiv:2001.02231 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

Brough S, Collins C, Demarco R, Ferguson HC, Galaz G, Holwerda B, Martinez-Lombilla C, Mihos C, Montes M (2020) The Vera Rubin Observatory Legacy Survey of Space and Time and the Low Surface Brightness Universe. arXiv e-prints arXiv:2001.11067. arXiv:2001.11067 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

Cameron AD, Champion DJ, Bailes M, Balakrishnan V, Barr ED, Bassa CG, Bates S, Bhandari S, Bhat NDR, Burgay M, et al. (2020) The High Time Resolution Universe Pulsar Survey - XVI. Discovery and timing of 40 pulsars from the southern Galactic plane. MNRAS 493(1):1063–1087. https://doi.org/10.1093/mnras/staa039 . arXiv:2001.01823 [astro-ph.HE]

Original

2001

Earlier work this paper cites.

Chon S, Omukai K (2020) Supermassive star formation via super competitive accretion in slightly metal-enriched clouds. MNRAS https://doi.org/10.1093/mnras/staa863 . arXiv:2001.06491 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

De Rosa A, Vignali C, Bogdanović T, Capelo PR, Charisi M, Dotti M, Husemann B, Lusso E, Mayer L, Paragi Z, et al. (2019b) The quest for dual and binary supermassive black holes: A multi-messenger view. New A Rev. 86:101525. https://doi.org/10.1016/j.newar.2020.101525 . arXiv:2001.06293 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

Ebisuzaki T, Makino J, Tsuru TG, Funato Y, Portegies Zwart S, Hut P, McMillan S, Matsushita S, Matsumoto H, Kawabe R (2001) Missing Link Found? The “Runaway” Path to Supermassive Black Holes. ApJ 562(1):L19–L22. https://doi.org/10.1086/338118 . arXiv:astro-ph/0106252 [astro-ph]

2001

Earlier work this paper cites.

Freitag M (2001) Monte Carlo cluster simulations to determine the rate of compact star inspiralling to a central galactic black hole. Classical and Quantum Gravity 18(19):4033–4038. https://doi.org/10.1088/0264-9381/18/19/309 . arXiv:astro-ph/0107193 [astro-ph]

2001

Earlier work this paper cites.

Gaspari M, Tombesi F, Cappi M (2020) Linking macro-, meso- and microscales in multiphase AGN feeding and feedback. Nature Astronomy 4:10–13. https://doi.org/10.1038/s41550-019-0970-1 . arXiv:2001.04985 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

Haiman Z, Loeb A (2001) What Is the Highest Plausible Redshift of Luminous Quasars? ApJ 552(2):459–463. https://doi.org/10.1086/320586 . arXiv:astro-ph/0011529 [astro-ph]

2001

Earlier work this paper cites.

Heinämäki P (2001) Symmetry of black hole ejections in mergers of galaxies. A&A 371:795–805. https://doi.org/10.1051/0004-6361:20010460

2001

Earlier work this paper cites.

Hilditch RW (2001) An Introduction to Close Binary Stars

2001

Earlier work this paper cites.

Izquierdo-Villalba D, Bonoli S, Dotti M, Sesana A, Rosas-Guevara Y, Spinoso D (2020) From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments. MNRAS 495(4):4681–4706. https://doi.org/10.1093/mnras/staa1399 . arXiv:2001.10548 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

Juett AM, Psaltis D, Chakrabarty D (2001) Ultracompact X-Ray Binaries with Neon-rich Degenerate Donors. ApJ 560(1):L59–L63. https://doi.org/10.1086/324225 . arXiv:astro-ph/0108102 [astro-ph]

2001

Earlier work this paper cites.

Koliopanos F, Peault M, Vasilopoulos G, Webb N (2020) The chemical composition of the accretion disk and donor star in Ultra Compact X-ray Binaries: A comprehensive X-ray analysis. arXiv e-prints arXiv:2001.00716. arXiv:2001.00716 [astro-ph.HE]

Original

2001

Earlier work this paper cites.

Kroupa P (2001) On the variation of the initial mass function. MNRAS 322(2):231–246. https://doi.org/10.1046/j.1365-8711.2001.04022.x . arXiv:astro-ph/0009005 [astro-ph]

2001

Earlier work this paper cites.

Kumamoto J, Fujii MS, Tanikawa A (2020) Merger rate density of binary black holes formed in open clusters. MNRAS 495(4):4268–4278. https://doi.org/10.1093/mnras/staa1440 . arXiv:2001.10690 [astro-ph.HE]

Original

2001

Earlier work this paper cites.

Lai D, Chernoff DF, Cordes JM (2001) Pulsar Jets: Implications for Neutron Star Kicks and Initial Spins. ApJ 549(2):1111–1118. https://doi.org/10.1086/319455 . arXiv:astro-ph/0007272 [astro-ph]

2001

Earlier work this paper cites.

Lim H, Rodriguez CL (2020) Relativistic three-body effects in hierarchical triples. Phys. Rev. D 102(6):064033. https://doi.org/10.1103/PhysRevD.102.064033 . arXiv:2001.03654 [astro-ph.HE]

Original

2001

Earlier work this paper cites.

Madau P, Rees MJ (2001) Massive Black Holes as Population III Remnants. ApJ 551(1):L27–L30. https://doi.org/10.1086/319848 . arXiv:astro-ph/0101223 [astro-ph]

2001

Earlier work this paper cites.

Merritt D (2001) Brownian Motion of a Massive Binary. ApJ 556(1):245–264. https://doi.org/10.1086/321550 . arXiv:astro-ph/0012264 [astro-ph]

2001

Earlier work this paper cites.

Milosavljević M, Merritt D (2001) Formation of Galactic Nuclei. ApJ 563(1):34–62. https://doi.org/10.1086/323830 . arXiv:astro-ph/0103350 [astro-ph]

2001

Earlier work this paper cites.

Neumayer N, Seth A, Böker T (2020) Nuclear star clusters. A&A Rev. 28(1):4. https://doi.org/10.1007/s00159-020-00125-0 . arXiv:2001.03626 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

O’Leary JA, Moster BP, Naab T, Somerville RS (2021) EMERGE: empirical predictions of galaxy merger rates since z ∼ \sim 6. MNRAS 501(3):3215–3237. https://doi.org/10.1093/mnras/staa3746 . arXiv:2001.02687

Original

2001

Earlier work this paper cites.

Pfister H, Dotti M, Laigle C, Dubois Y, Volonteri M (2020) Real galaxy mergers from galaxy pair catalogues. MNRAS 493(1):922–929. https://doi.org/10.1093/mnras/staa227 . arXiv:2001.02461 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

Ruiter AJ (2020) Type Ia supernova sub-classes and progenitor origin. IAU Symposium 357:1–15. https://doi.org/10.1017/S1743921320000587 . arXiv:2001.02947 [astro-ph.SR]

Original

2001

Earlier work this paper cites.

Ryu T, Krolik J, Piran T, Noble SC (2020) Tidal Disruptions of Main-sequence Stars. II. Simulation Methodology and Stellar Mass Dependence of the Character of Full Tidal Disruptions. ApJ 904(2):99. https://doi.org/10.3847/1538-4357/abb3cd . arXiv:2001.03502 [astro-ph.HE]

Original

2001

Earlier work this paper cites.

Safarzadeh M, Ramirez-Ruiz E, Berger E (2020b) Does GW190425 Require an Alternative Formation Pathway than a Fast-merging Channel? ApJ 900(1):13. https://doi.org/10.3847/1538-4357/aba596 . arXiv:2001.04502 [astro-ph.HE]

Original

2001

Earlier work this paper cites.

Schneider R, Ferrari V, Matarrese S, Portegies Zwart SF (2001) Low-frequency gravitational waves from cosmological compact binaries. MNRAS 324(4):797–810. https://doi.org/10.1046/j.1365-8711.2001.04217.x . arXiv:astro-ph/0002055 [astro-ph]

2001

Earlier work this paper cites.

Shen X, Hopkins PF, Faucher-Giguère CA, Alexander DM, Richards GT, Ross NP, Hickox RC (2020) The bolometric quasar luminosity function at z = 0-7. MNRAS 495(3):3252–3275. https://doi.org/10.1093/mnras/staa1381 . arXiv:2001.02696 [astro-ph.GA]

Original

2001

Earlier work this paper cites.

Springel V, White SDM, Tormen G, Kauffmann G (2001) Populating a cluster of galaxies - I. Results at [formmu2]z=0. MNRAS 328(3):726–750. https://doi.org/10.1046/j.1365-8711.2001.04912.x . arXiv:astro-ph/0012055 [astro-ph]

2001

Earlier work this paper cites.

Stadel JG (2001) Cosmological N-body simulations and their analysis. PhD thesis, UNIVERSITY OF WASHINGTON

2001

Earlier work this paper cites.

Tauris TM, Dewi JDM (2001) Research Note On the binding energy parameter of common envelope evolution. Dependency on the definition of the stellar core boundary during spiral-in. A&A 369:170–173. https://doi.org/10.1051/0004-6361:20010099 . arXiv:astro-ph/0101530 [astro-ph]

2001

Earlier work this paper cites.

Torres-Orjuela A, Chen X, Amaro-Seoane P (2020b) Phase shift of gravitational waves induced by aberration. Phys. Rev. D 101(8):083028. https://doi.org/10.1103/PhysRevD.101.083028 . arXiv:2001.00721 [astro-ph.HE]

Original

2001

Earlier work this paper cites.

Ullio P, Zhao H, Kamionkowski M (2001) Dark-matter spike at the galactic center? Phys. Rev. D 64(4):043504. https://doi.org/10.1103/PhysRevD.64.043504 . arXiv:astro-ph/0101481 [astro-ph]

2001

Earlier work this paper cites.

van Putten MH (2001) Proposed Source of Gravitational Radiation from a Torus around a Black Hole. Phys. Rev. Lett. 87(9):091101. https://doi.org/10.1103/PhysRevLett.87.091101 . arXiv:astro-ph/0107007 [astro-ph]

2001

Earlier work this paper cites.

Vigna-Gómez A, MacLeod M, Neijssel CJ, Broekgaarden FS, Justham S, Howitt G, de Mink SE, Vinciguerra S, Mandel I (2020) Common-Envelope Episodes that lead to Double Neutron Star formation. arXiv e-prints arXiv:2001.09829. arXiv:2001.09829 [astro-ph.SR]

Original

2001

Earlier work this paper cites.

Abel T, Bryan GL, Norman ML (2002) The Formation of the First Star in the Universe. Science 295:93–98. https://doi.org/10.1126/science.1063991 . arXiv:astro-ph/0112088

2002

Earlier work this paper cites.

Arca Sedda M (2020a) Birth, Life, and Death of Black Hole Binaries around Supermassive Black Holes: Dynamical Evolution of Gravitational Wave Sources. ApJ 891(1):47. https://doi.org/10.3847/1538-4357/ab723b . arXiv:2002.04037 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Armitage PJ, Natarajan P (2002) Accretion during the Merger of Supermassive Black Holes. ApJ 567(1):L9–L12. https://doi.org/10.1086/339770 . arXiv:astro-ph/0201318 [astro-ph]

2002

Earlier work this paper cites.

Athanassoula E (2002) Formation and Evolution of Bars in Disc Galaxies. In: Athanassoula E, Bosma A, Mujica R (eds) Disks of Galaxies: Kinematics, Dynamics and Peturbations. Astronomical Society of the Pacific Conference Series, vol 275. pp 141–152. arXiv:astro-ph/0209438 [astro-ph]

2002

Earlier work this paper cites.

Belczynski K, Kalogera V, Bulik T (2002) A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties. ApJ 572(1):407–431. https://doi.org/10.1086/340304 . arXiv:astro-ph/0111452 [astro-ph]

2002

Earlier work this paper cites.

Blaes O, Lee MH, Socrates A (2002) The Kozai Mechanism and the Evolution of Binary Supermassive Black Holes. ApJ 578(2):775–786. https://doi.org/10.1086/342655 . arXiv:astro-ph/0203370 [astro-ph]

2002

Earlier work this paper cites.

Bonetti M, Bortolas E, Lupi A, Dotti M, Raimundo SI (2020a) Dynamical friction-driven orbital circularization in rotating discs: a semi-analytical description. MNRAS 494(2):3053–3059. https://doi.org/10.1093/mnras/staa964 . arXiv:2002.04621 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Brown WR, Kilic M, Kosakowski A, Andrews JJ, Heinke CO, Agüeros MA, Camilo F, Gianninas A, Hermes JJ, Kenyon SJ (2020b) The ELM Survey. VIII. Ninety-eight Double White Dwarf Binaries. ApJ 889(1):49. https://doi.org/10.3847/1538-4357/ab63cd . arXiv:2002.00064 [astro-ph.SR]

Original

2002

Earlier work this paper cites.

Carr B, Kohri K, Sendouda Y, Yokoyama J (2021) Constraints on primordial black holes. Reports on Progress in Physics 84(11):116902. https://doi.org/10.1088/1361-6633/ac1e31 . arXiv:2002.12778 [astro-ph.CO]

Original

2002

Earlier work this paper cites.

Chruślińska M, Jeřábková T, Nelemans G, Yan Z (2020) The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history. A&A 636:A10. https://doi.org/10.1051/0004-6361/202037688 . arXiv:2002.11122 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Contopoulos G (2002) Order and chaos in dynamical astronomy. Springer

2002

Earlier work this paper cites.

du Buisson L, Marchant P, Podsiadlowski P, Kobayashi C, Abdalla FB, Taylor P, Mandel I, de Mink SE, Moriya TJ, Langer N (2020) Cosmic Rates of Black Hole Mergers and Pair-Instability Supernovae from Chemically Homogeneous Binary Evolution. arXiv e-prints arXiv:2002.11630. arXiv:2002.11630 [astro-ph.HE]

Original

2002

Earlier work this paper cites.

Dunn G, Holley-Bockelmann K, Bellovary J (2020) The Role of Gravitational Recoil in the Assembly of Massive Black Hole Seeds. ApJ 896(1):72. https://doi.org/10.3847/1538-4357/ab7cd2 . arXiv:2002.04740 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Frank J, King A, Raine DJ (2002) Accretion Power in Astrophysics: Third Edition

2002

Earlier work this paper cites.

Generozov A, Madigan AM (2020) The Hills Mechanism and the Galactic Center S-stars. ApJ 896(2):137. https://doi.org/10.3847/1538-4357/ab94bc . arXiv:2002.10547 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Horton MA, Hardcastle MJ, Read SC, Krause MGH (2020) A Markov chain Monte Carlo approach for measurement of jet precession in radio-loud active galactic nuclei. MNRAS 493(3):3911–3919. https://doi.org/10.1093/mnras/staa429 . arXiv:2002.04966 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Hurley JR, Tout CA, Pols OR (2002) Evolution of binary stars and the effect of tides on binary populations. MNRAS 329(4):897–928. https://doi.org/10.1046/j.1365-8711.2002.05038.x . arXiv:astro-ph/0201220 [astro-ph]

2002

Earlier work this paper cites.

Kavanagh BJ, Nichols DA, Bertone G, Gaggero D (2020) Detecting dark matter around black holes with gravitational waves: Effects of dark-matter dynamics on the gravitational waveform. Phys. Rev. D 102(8):083006. https://doi.org/10.1103/PhysRevD.102.083006 . arXiv:2002.12811 [gr-qc]

Original

2002

Earlier work this paper cites.

Korol V, Toonen S, Klein A, Belokurov V, Vincenzo F, Buscicchio R, Gerosa D, Moore CJ, Roebber E, Rossi EM, et al. (2020) Populations of double white dwarfs in Milky Way satellites and their detectability with LISA. A&A 638:A153. https://doi.org/10.1051/0004-6361/202037764 . arXiv:2002.10462 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Kupfer T, Bauer EB, Marsh TR, van Roestel J, Bellm EC, Burdge KB, Coughlin MW, Fuller J, et al (2020b) The First Ultracompact Roche Lobe-Filling Hot Subdwarf Binary. ApJ 891(1):45. https://doi.org/10.3847/1538-4357/ab72ff . arXiv:2002.01485 [astro-ph.SR]

Original

2002

Earlier work this paper cites.

Marsh TR, Steeghs D (2002) V407 Vul: a direct impact accretor. MNRAS 331(1):L7–L11. https://doi.org/10.1046/j.1365-8711.2002.05346.x . arXiv:astro-ph/0201309 [astro-ph]

2002

Earlier work this paper cites.

Maxted PFL, Marsh TR, Moran CKJ (2002) The mass ratio distribution of short-period double degenerate stars. MNRAS 332(3):745–753. https://doi.org/10.1046/j.1365-8711.2002.05368.x . arXiv:astro-ph/0201411 [astro-ph]

2002

Earlier work this paper cites.

McKernan B, Ford KES, O’Shaughnessy R (2020a) Black hole, neutron star, and white dwarf merger rates in AGN discs. MNRAS 498(3):4088–4094. https://doi.org/10.1093/mnras/staa2681 . arXiv:2002.00046 [astro-ph.HE]

Original

2002

Earlier work this paper cites.

Merritt D, Milosavljević M, Verde L, Jimenez R (2002) Dark Matter Spikes and Annihilation Radiation from the Galactic Center. Phys. Rev. Lett. 88(19):191301. https://doi.org/10.1103/PhysRevLett.88.191301 . arXiv:astro-ph/0201376 [astro-ph]

2002

Earlier work this paper cites.

Miller MC, Hamilton DP (2002b) Production of intermediate-mass black holes in globular clusters. MNRAS 330(1):232–240. https://doi.org/10.1046/j.1365-8711.2002.05112.x . arXiv:astro-ph/0106188 [astro-ph]

2002

Earlier work this paper cites.

Omukai K, Inutsuka Si (2002) An upper limit on the mass of a primordial star due to the formation of an Hii region: the effect of ionizing radiation force. MNRAS 332(1):59–64. https://doi.org/10.1046/j.1365-8711.2002.05276.x . arXiv:astro-ph/0112345 [astro-ph]

2002

Earlier work this paper cites.

Phillips SN, Podsiadlowski P (2002) Irradiation pressure effects in close binary systems. MNRAS 337(2):431–444. https://doi.org/10.1046/j.1365-8711.2002.05886.x . arXiv:astro-ph/0109304 [astro-ph]

2002

Earlier work this paper cites.

Podsiadlowski P, Rappaport S, Pfahl ED (2002) Evolutionary Sequences for Low- and Intermediate-Mass X-Ray Binaries. ApJ 565(2):1107–1133. https://doi.org/10.1086/324686 . arXiv:astro-ph/0107261 [astro-ph]

2002

Earlier work this paper cites.

Portegies Zwart SF, McMillan SLW (2002) The Runaway Growth of Intermediate-Mass Black Holes in Dense Star Clusters. ApJ 576(2):899–907. https://doi.org/10.1086/341798 . arXiv:astro-ph/0201055 [astro-ph]

2002

Earlier work this paper cites.

Roebber E, Buscicchio R, Vecchio A, Moore CJ, Klein A, Korol V, Toonen S, Gerosa D, Goldstein J, Gaebel SM, et al. (2020) Milky Way Satellites Shining Bright in Gravitational Waves. ApJ 894(2):L15. https://doi.org/10.3847/2041-8213/ab8ac9 . arXiv:2002.10465 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Serpico PD, Poulin V, Inman D, Kohri K (2020) Cosmic microwave background bounds on primordial black holes including dark matter halo accretion. Phys Rev Res 2(2):023204. https://doi.org/10.1103/PhysRevResearch.2.023204 . arXiv:2002.10771 [astro-ph.CO]

Original

2002

Earlier work this paper cites.

Takekawa S, Oka T, Iwata Y, Tsujimoto S, Nomura M (2020) The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center. ApJ 890(2):167. https://doi.org/10.3847/1538-4357/ab6f6f . arXiv:2002.05173 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Tanaka H, Takeuchi T, Ward WR (2002) Three-Dimensional Interaction between a Planet and an Isothermal Gaseous Disk. I. Corotation and Lindblad Torques and Planet Migration. ApJ 565(2):1257–1274. https://doi.org/10.1086/324713

2002

Earlier work this paper cites.

Toyouchi D, Hosokawa T, Sugimura K, Kuiper R (2020) Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down? MNRAS 496(2):1909–1921. https://doi.org/10.1093/mnras/staa1338 . arXiv:2002.08017 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Trebitsch M, Dubois Y, Volonteri M, Pfister H, Cadiou C, Katz H, Rosdahl J, Kimm T, Pichon C, Beckmann RS, et al. (2020) The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters. arXiv e-prints arXiv:2002.04045. arXiv:2002.04045 [astro-ph.GA]

Original

2002

Earlier work this paper cites.

Tremaine S, Gebhardt K, Bender R, Bower G, Dressler A, Faber SM, Filippenko AV, Green R, Grillmair C, Ho LC, et al. (2002) The Slope of the Black Hole Mass versus Velocity Dispersion Correlation. ApJ 574(2):740–753. https://doi.org/10.1086/341002 . arXiv:astro-ph/0203468 [astro-ph]

2002

Earlier work this paper cites.

Unal C, Loeb A (2020) On Spin Dependence of the Fundamental Plane of Black Hole Activity. Mon Not Roy Astron Soc 495(1):278–284. https://doi.org/10.1093/mnras/staa1119 . arXiv:2002.11778 [astro-ph.HE]

Original

2002

Earlier work this paper cites.

van Putten MHPM (2002) LIGO/VIRGO Searches for Gravitational Radiation in Hypernovae. ApJ 575(2):L71–L74. https://doi.org/10.1086/342781 . arXiv:astro-ph/0207242 [astro-ph]

2002

Earlier work this paper cites.

Varma V, Isi M, Biscoveanu S (2020) Extracting the Gravitational Recoil from Black Hole Merger Signals. Phys. Rev. Lett. 124(10):101104. https://doi.org/10.1103/PhysRevLett.124.101104 . arXiv:2002.00296 [gr-qc]

Original

2002

Earlier work this paper cites.

Wu K, Cropper M, Ramsay G, Sekiguchi K (2002) An electrically powered binary star? MNRAS 331(1):221–227. https://doi.org/10.1046/j.1365-8711.2002.05190.x . arXiv:astro-ph/0111358 [astro-ph]

2002

Earlier work this paper cites.

Yu Q (2002) Evolution of massive binary black holes. MNRAS 331(4):935–958. https://doi.org/10.1046/j.1365-8711.2002.05242.x . arXiv:astro-ph/0109530 [astro-ph]

2002

Earlier work this paper cites.

Yu Q, Tremaine S (2002) Observational constraints on growth of massive black holes. MNRAS 335(4):965–976. https://doi.org/10.1046/j.1365-8711.2002.05532.x . arXiv:astro-ph/0203082 [astro-ph]

2002

Earlier work this paper cites.

Arca Sedda M (2020b) Dissecting the properties of neutron star-black hole mergers originating in dense star clusters. Communications Physics 3(1):43. https://doi.org/10.1038/s42005-020-0310-x . arXiv:2003.02279 [astro-ph.GA]

Original

2003

Earlier work this paper cites.

Arca Sedda M, Mapelli M, Spera M, Benacquista M, Giacobbo N (2020b) Fingerprints of Binary Black Hole Formation Channels Encoded in the Mass and Spin of Merger Remnants. ApJ 894(2):133. https://doi.org/10.3847/1538-4357/ab88b2 . arXiv:2003.07409 [astro-ph.GA]

Original

2003

Earlier work this paper cites.

Chabrier G (2003) Galactic Stellar and Substellar Initial Mass Function. PASP 115(809):763–795. https://doi.org/10.1086/376392 . arXiv:astro-ph/0304382 [astro-ph]

2003

Earlier work this paper cites.

Chatterjee P, Hernquist L, Loeb A (2003) Effects of Wandering on the Coalescence of Black Hole Binaries in Galactic Centers. ApJ 592(1):32–41. https://doi.org/10.1086/375552 . arXiv:astro-ph/0302573 [astro-ph]

2003

Earlier work this paper cites.

Cornish NJ, Larson SL (2003) LISA data analysis: Source identification and subtraction. Phys. Rev. D 67(10):103001. https://doi.org/10.1103/PhysRevD.67.103001 . arXiv:astro-ph/0301548 [astro-ph]

2003

Earlier work this paper cites.

De Luca V, Franciolini G, Pani P, Riotto A (2020) Constraints on Primordial Black Holes: the Importance of Accretion. Phys Rev D 102(4):043505. https://doi.org/10.1103/PhysRevD.102.043505 . arXiv:2003.12589 [astro-ph.CO]

Original

2003

Earlier work this paper cites.

Dewi JDM, Pols OR (2003) The late stages of evolution of helium star-neutron star binaries and the formation of double neutron star systems. MNRAS 344(2):629–643. https://doi.org/10.1046/j.1365-8711.2003.06844.x . arXiv:astro-ph/0306066 [astro-ph]

2003

Earlier work this paper cites.

Fan X, Strauss MA, Schneider DP, Becker RH, White RL, Haiman Z, Gregg M, Pentericci L, Grebel EK, Narayanan VK, et al. (2003) A Survey of z>5.7 Quasars in the Sloan Digital Sky Survey. II. Discovery of Three Additional Quasars at z>6. AJ 125(4):1649–1659. https://doi.org/10.1086/368246 . arXiv:astro-ph/0301135 [astro-ph]

2003

Earlier work this paper cites.

Farmer AJ, Phinney ES (2003) The gravitational wave background from cosmological compact binaries. MNRAS 346(4):1197–1214. https://doi.org/10.1111/j.1365-2966.2003.07176.x . arXiv:astro-ph/0304393 [astro-ph]

2003

Earlier work this paper cites.

Goicovic FG, Cuadra J, Sesana A, Stasyszyn F, Amaro-Seoane P, Tanaka TL (2016) Infalling clouds on to supermassive black hole binaries - I. Formation of discs, accretion and gas dynamics. MNRAS 455(2):1989–2003. https://doi.org/10.1093/mnras/stv2470 . arXiv:1507.05596 [astro-ph.HE]

Original

2003

Earlier work this paper cites.

Goodman J (2003) Self-gravity and quasi-stellar object discs. MNRAS 339(4):937–948. https://doi.org/10.1046/j.1365-8711.2003.06241.x . arXiv:astro-ph/0201001 [astro-ph]

2003

Earlier work this paper cites.

Graham AW, Erwin P, Trujillo I, Asensio Ramos A (2003) A New Empirical Model for the Structural Analysis of Early-Type Galaxies, and A Critical Review of the Nuker Model. AJ 125(6):2951–2963. https://doi.org/10.1086/375320 . arXiv:astro-ph/0306023 [astro-ph]

2003

Earlier work this paper cites.

Hansen BMS, Milosavljević M (2003) The Need for a Second Black Hole at the Galactic Center. ApJ 593(2):L77–L80. https://doi.org/10.1086/378182 . arXiv:astro-ph/0306074 [astro-ph]

2003

Earlier work this paper cites.

Heger A, Fryer CL, Woosley SE, Langer N, Hartmann DH (2003) How Massive Single Stars End Their Life. ApJ 591:288–300. https://doi.org/10.1086/375341 . arXiv:astro-ph/0212469

2003

Earlier work this paper cites.

Heggie D, Hut P (2003) The Gravitational Million-Body Problem: A Multidisciplinary Approach to Star Cluster Dynamics

2003

Earlier work this paper cites.

Heinke CO, Grindlay JE, Lugger PM, Cohn HN, Edmonds PD, Lloyd DA, Cool AM (2003) Analysis of the Quiescent Low-Mass X-Ray Binary Population in Galactic Globular Clusters. ApJ 598(1):501–515. https://doi.org/10.1086/378885 . arXiv:astro-ph/0305445 [astro-ph]

2003

Earlier work this paper cites.

Hughes SA, Blandford RD (2003) Black Hole Mass and Spin Coevolution by Mergers. ApJ 585(2):L101–L104. https://doi.org/10.1086/375495 . arXiv:astro-ph/0208484 [astro-ph]

2003

Earlier work this paper cites.

Ivanova N, Belczynski K, Kalogera V, Rasio FA, Taam RE (2003) The Role of Helium Stars in the Formation of Double Neutron Stars. ApJ 592(1):475–485. https://doi.org/10.1086/375578 . arXiv:astro-ph/0210267 [astro-ph]

2003

Earlier work this paper cites.

Kerr M, Reardon DJ, Hobbs G, Shannon RM, Manchester RN, Dai S, Russell CJ, Zhang S, van Straten W, Osłowski S, et al. (2020) The Parkes Pulsar Timing Array project: second data release. PASA 37:e020. https://doi.org/10.1017/pasa.2020.11 . arXiv:2003.09780 [astro-ph.IM]

Original

2003

Earlier work this paper cites.

Kim C, Kalogera V, Lorimer DR (2003) The Probability Distribution of Binary Pulsar Coalescence Rates. I. Double Neutron Star Systems in the Galactic Field. ApJ 584(2):985–995. https://doi.org/10.1086/345740 . arXiv:astro-ph/0207408 [astro-ph]

2003

Earlier work this paper cites.

King A (2003) Black Holes, Galaxy Formation, and the M BH

2003

Earlier work this paper cites.

Kuroda T, Arcones A, Takiwaki T, Kotake K (2020) Magnetorotational Explosion of a Massive Star Supported by Neutrino Heating in General Relativistic Three-dimensional Simulations. ApJ 896(2):102. https://doi.org/10.3847/1538-4357/ab9308 . arXiv:2003.02004 [astro-ph.HE]

Original

2003

Earlier work this paper cites.

Kuulkers E, den Hartog PR, in’t Zand JJM, Verbunt FWM, Harris WE, Cocchi M (2003) Photospheric radius expansion X-ray bursts as standard candles. A&A 399:663–680. https://doi.org/10.1051/0004-6361:20021781 . arXiv:astro-ph/0212028 [astro-ph]

2003

Earlier work this paper cites.

Levin Y, Beloborodov AM (2003) Stellar Disk in the Galactic Center: A Remnant of a Dense Accretion Disk? ApJ 590(1):L33–L36. https://doi.org/10.1086/376675 . arXiv:astro-ph/0303436 [astro-ph]

2003

Earlier work this paper cites.

Milosavljević M, Merritt D (2003) Long-Term Evolution of Massive Black Hole Binaries. ApJ 596(2):860–878. https://doi.org/10.1086/378086 . arXiv:astro-ph/0212459 [astro-ph]

2003

Earlier work this paper cites.

Oh SP, Haiman Z (2003) Fossil H II regions: self-limiting star formation at high redshift. MNRAS 346(2):456–472. https://doi.org/10.1046/j.1365-2966.2003.07103.x . arXiv:astro-ph/0307135 [astro-ph]

2003

Earlier work this paper cites.

Omukai K, Palla F (2003) Formation of the First Stars by Accretion. ApJ 589(2):677–687. https://doi.org/10.1086/374810 . arXiv:astro-ph/0302345 [astro-ph]

2003

Earlier work this paper cites.

Podsiadlowski P, Rappaport S, Han Z (2003) On the formation and evolution of black hole binaries. MNRAS 341(2):385–404. https://doi.org/10.1046/j.1365-8711.2003.06464.x . arXiv:astro-ph/0207153 [astro-ph]

2003

Earlier work this paper cites.

Rastello S, Mapelli M, Di Carlo UN, Giacobbo N, Santoliquido F, Spera M, Ballone A, Iorio G (2020) Dynamics of black hole-neutron star binaries in young star clusters. MNRAS 497(2):1563–1570. https://doi.org/10.1093/mnras/staa2018 . arXiv:2003.02277 [astro-ph.HE]

Original

2003

Earlier work this paper cites.

Reynolds CS, Nowak MA (2003) Fluorescent iron lines as a probe of astrophysical black hole systems. Phys. Rep. 377(6):389–466. https://doi.org/10.1016/S0370-1573(02)00584-7 . arXiv:astro-ph/0212065 [astro-ph]

2003

Earlier work this paper cites.

Ricarte A, Tremmel M, Natarajan P, Quinn T (2020) A Link between Ram Pressure Stripping and Active Galactic Nuclei. ApJ 895(1):L8. https://doi.org/10.3847/2041-8213/ab9022 . arXiv:2003.05950 [astro-ph.GA]

Original

2003

Earlier work this paper cites.

Sigurdsson S, Richer HB, Hansen BM, Stairs IH, Thorsett SE (2003) A Young White Dwarf Companion to Pulsar B1620-26: Evidence for Early Planet Formation. Science 301(5630):193–196. https://doi.org/10.1126/science.1086326 . arXiv:astro-ph/0307339 [astro-ph]

2003

Earlier work this paper cites.

Sirko E, Goodman J (2003) Spectral energy distributions of marginally self-gravitating quasi-stellar object discs. MNRAS 341(2):501–508. https://doi.org/10.1046/j.1365-8711.2003.06431.x , URL http://dx.doi.org/10.1046/j.1365-8711.2003.06431.x

2003

Earlier work this paper cites.

Soker N, Tylenda R (2003) Main-Sequence Stellar Eruption Model for V838 Monocerotis. ApJ 582(2):L105–L108. https://doi.org/10.1086/367759 . arXiv:astro-ph/0210463 [astro-ph]

2003

Earlier work this paper cites.

Souza Lima R, Mayer L, Capelo PR, Bortolas E, Quinn TR (2020) The Erratic Path to Coalescence of LISA Massive Black Hole Binaries in Subparsec-resolution Simulations of Smooth Circumnuclear Gas Disks. ApJ 899(2):126. https://doi.org/10.3847/1538-4357/aba624 . arXiv:2003.13789 [astro-ph.GA]

Original

2003

Earlier work this paper cites.

Vinciguerra S, Neijssel CJ, Vigna-Gómez A, Mandel I, Podsiadlowski P, Maccarone TJ, Nicholl M, Kingdon S, Perry A, Salemi F (2020) Be X-ray binaries in the SMC as indicators of mass-transfer efficiency. MNRAS 498(4):4705–4720. https://doi.org/10.1093/mnras/staa2177 . arXiv:2003.00195 [astro-ph.HE]

Original

2003

Earlier work this paper cites.

Voss R, Tauris TM (2003) Galactic distribution of merging neutron stars and black holes - prospects for short gamma-ray burst progenitors and LIGO/VIRGO. MNRAS 342(4):1169–1184. https://doi.org/10.1046/j.1365-8711.2003.06616.x . arXiv:astro-ph/0303227 [astro-ph]

2003

Earlier work this paper cites.

Wadsley JW, Stadel J, Quinn T (2004) Gasoline: a flexible, parallel implementation of TreeSPH. New A 9(2):137–158. https://doi.org/10.1016/j.newast.2003.08.004 . arXiv:astro-ph/0303521 [astro-ph]

2003

Earlier work this paper cites.

Wen L (2003) On the Eccentricity Distribution of Coalescing Black Hole Binaries Driven by the Kozai Mechanism in Globular Clusters. ApJ 598(1):419–430. https://doi.org/10.1086/378794 . arXiv:astro-ph/0211492 [astro-ph]

2003

Earlier work this paper cites.

Wilhelm MJC, Korol V, Rossi EM, D’Onghia E (2020) The Milky Way’s bar structural properties from gravitational waves. arXiv e-prints arXiv:2003.11074. arXiv:2003.11074 [astro-ph.GA]

Original

2003

Earlier work this paper cites.

Yoshida N, Abel T, Hernquist L, Sugiyama N (2003) Simulations of Early Structure Formation: Primordial Gas Clouds. ApJ 592:645–663. https://doi.org/10.1086/375810 . arXiv:astro-ph/0301645

2003

Earlier work this paper cites.

Yu Q, Tremaine S (2003) Ejection of Hypervelocity Stars by the (Binary) Black Hole in the Galactic Center. ApJ 599(2):1129–1138. https://doi.org/10.1086/379546 . arXiv:astro-ph/0309084 [astro-ph]

2003

Earlier work this paper cites.

Abuter R, Amorim A, Bauböck M, Berger JP, Bonnet H, Brand ner W, Cardoso V, Clénet Y, de Zeeuw PT, Dexter J, et al. (2020) Detection of the Schwarzschild precession in the orbit of the star S2 near the Galactic centre massive black hole. A&A 636:L5. https://doi.org/10.1051/0004-6361/202037813 . arXiv:2004.07187 [astro-ph.GA]

Original

2004

Earlier work this paper cites.

Baldry IK, Glazebrook K, Brinkmann J, Ivezić Ž, Lupton RH, Nichol RC, Szalay AS (2004) Quantifying the Bimodal Color-Magnitude Distribution of Galaxies. ApJ 600(2):681–694. https://doi.org/10.1086/380092 . arXiv:astro-ph/0309710 [astro-ph]

2004

Earlier work this paper cites.

Banerjee S (2021) Stellar-mass black holes in young massive and open stellar clusters - IV. Updated stellar-evolutionary and black hole spin models and comparisons with the LIGO-Virgo O1/O2 merger-event data. MNRAS 500(3):3002–3026. https://doi.org/10.1093/mnras/staa2392 . arXiv:2004.07382 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Boylan-Kolchin M, Ma CP, Quataert E (2004) Core Formation in Galactic Nuclei due to Recoiling Black Holes. ApJ 613(1):L37–L40. https://doi.org/10.1086/425073 . arXiv:astro-ph/0407488 [astro-ph]

2004

Earlier work this paper cites.

Brown WR, Kilic M, Bédard A, Kosakowski A, Bergeron P (2020a) A 1201 s Orbital Period Detached Binary: The First Double Helium Core White Dwarf LISA Verification Binary. ApJ 892(2):L35. https://doi.org/10.3847/2041-8213/ab8228 . arXiv:2004.00641 [astro-ph.SR]

Original

2004

Earlier work this paper cites.

Büning A, Ritter H (2004) Long-term evolution of compact binaries with irradiation feedback. A&A 423:281–299. https://doi.org/10.1051/0004-6361:20035678 . arXiv:astro-ph/0403306 [astro-ph]

2004

Earlier work this paper cites.

Di Carlo UN, Mapelli M, Giacobbo N, Spera M, Bouffanais Y, Rastello S, Santoliquido F, Pasquato M, Ballone Ar, Trani AA, et al. (2020b) Binary black holes in young star clusters: the impact of metallicity. MNRAS 498(1):495–506. https://doi.org/10.1093/mnras/staa2286 . arXiv:2004.09525 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Duechting N (2004) Supermassive black holes from primordial black hole seeds. Phys Rev D 70:064015. https://doi.org/10.1103/PhysRevD.70.064015 . arXiv:astro-ph/0406260

2004

Earlier work this paper cites.

Gair JR, Barack L, Creighton T, Cutler C, Larson SL, Phinney ES, Vallisneri M (2004) Event rate estimates for LISA extreme mass ratio capture sources. Classical and Quantum Gravity 21(20):S1595–S1606. https://doi.org/10.1088/0264-9381/21/20/003 . arXiv:gr-qc/0405137 [gr-qc]

2004

Earlier work this paper cites.

Gammie CF, Shapiro SL, McKinney JC (2004) Black Hole Spin Evolution. ApJ 602(1):312–319. https://doi.org/10.1086/380996 . arXiv:astro-ph/0310886 [astro-ph]

2004

Earlier work this paper cites.

Gerosa D, Rosotti G, Barbieri R (2020) The Bardeen-Petterson effect in accreting supermassive black hole binaries: a systematic approach. MNRAS 496(3):3060–3075. https://doi.org/10.1093/mnras/staa1693 . arXiv:2004.02894 [astro-ph.GA]

Original

2004

Earlier work this paper cites.

Glanz H, Perets HB (2021) Simulations of common envelope evolution in triple systems: circumstellar case. MNRAS 500(2):1921–1932. https://doi.org/10.1093/mnras/staa3242 . arXiv:2004.00020 [astro-ph.SR]

Original

2004

Earlier work this paper cites.

Goodman J, Tan JC (2004) Supermassive Stars in Quasar Disks. ApJ 608(1):108–118. https://doi.org/10.1086/386360 . arXiv:astro-ph/0307361 [astro-ph]

2004

Earlier work this paper cites.

Graham AW (2004) Core Depletion from Coalescing Supermassive Black Holes. ApJ 613(1):L33–L36. https://doi.org/10.1086/424928 . arXiv:astro-ph/0503177 [astro-ph]

2004

Earlier work this paper cites.

Graziani L, Schneider R, Marassi S, Del Pozzo W, Mapelli M, Giacobbo N (2020) Cosmic archaeology with massive stellar black hole binaries. MNRAS 495(1):L81–L85. https://doi.org/10.1093/mnrasl/slaa063 . arXiv:2004.03603 [astro-ph.GA]

Original

2004

Earlier work this paper cites.

Gürkan MA, Freitag M, Rasio FA (2004) Formation of Massive Black Holes in Dense Star Clusters. I. Mass Segregation and Core Collapse. ApJ 604(2):632–652. https://doi.org/10.1086/381968 . arXiv:astro-ph/0308449 [astro-ph]

2004

Earlier work this paper cites.

Haiman Z (2004) Constraints from Gravitational Recoil on the Growth of Supermassive Black Holes at High Redshift. ApJ 613(1):36–40. https://doi.org/10.1086/422910 . arXiv:astro-ph/0404196 [astro-ph]

2004

Earlier work this paper cites.

Han WB, Zhong XY, Chen X, Xin S (2020) Very extreme mass-ratio bursts in the Galaxy and neighbouring galaxies in relation to space-borne detectors. MNRAS 498(1):L61–L65. https://doi.org/10.1093/mnrasl/slaa115 . arXiv:2004.04016 [gr-qc]

Original

2004

Earlier work this paper cites.

Izzard RG (2004) Nucleosynthesis In Binary Stars. PhD thesis, University of Cambridge

2004

Earlier work this paper cites.

Kiuchi K, Maeda KI (2004) Gravitational waves from a chaotic dynamical system. Phys. Rev. D 70(6):064036. https://doi.org/10.1103/PhysRevD.70.064036 . arXiv:gr-qc/0404124 [gr-qc]

2004

Earlier work this paper cites.

Kobayashi S, Laguna P, Phinney ES, Mészáros P (2004) Gravitational Waves and X-Ray Signals from Stellar Disruption by a Massive Black Hole. ApJ 615(2):855–865. https://doi.org/10.1086/424684 . arXiv:astro-ph/0404173 [astro-ph]

2004

Earlier work this paper cites.

Kormendy J (2004) The Stellar-Dynamical Search for Supermassive Black Holes in Galactic Nuclei. In: Ho LC (ed) Coevolution of Black Holes and Galaxies. p 1. arXiv:astro-ph/0306353 [astro-ph]

2004

Earlier work this paper cites.

Littenberg TB, Cornish NJ, Lackeos K, Robson T (2020) Global analysis of the gravitational wave signal from Galactic binaries. Phys. Rev. D 101(12):123021. https://doi.org/10.1103/PhysRevD.101.123021 . arXiv:2004.08464 [gr-qc]

Original

2004

Earlier work this paper cites.

Liu C, Shao L, Zhao J, Gao Y (2020) Multiband observation of LIGO/Virgo binary black hole mergers in the gravitational-wave transient catalog GWTC-1. MNRAS 496(1):182–196. https://doi.org/10.1093/mnras/staa1512 . arXiv:2004.12096 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Lyne AG, Burgay M, Kramer M, Possenti A, Manchester RN, Camilo F, McLaughlin MA, Lorimer DR, D’Amico N, Joshi BC, et al. (2004) A Double-Pulsar System: A Rare Laboratory for Relativistic Gravity and Plasma Physics. Science 303(5661):1153–1157. https://doi.org/10.1126/science.1094645 . arXiv:astro-ph/0401086 [astro-ph]

2004

Earlier work this paper cites.

Maguire K, Eracleous M, Jonker PG, MacLeod M, Rosswog S (2020) Tidal Disruptions of White Dwarfs: Theoretical Models and Observational Prospects. Space Sci. Rev. 216(3):39. https://doi.org/10.1007/s11214-020-00661-2 . arXiv:2004.00146 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Makino J, Funato Y (2004) Evolution of Massive Black Hole Binaries. ApJ 602(1):93–102. https://doi.org/10.1086/380917 . arXiv:astro-ph/0307327 [astro-ph]

2004

Earlier work this paper cites.

Marconi A, Risaliti G, Gilli R, Hunt LK, Maiolino R, Salvati M (2004) Local supermassive black holes, relics of active galactic nuclei and the X-ray background. MNRAS 351(1):169–185. https://doi.org/10.1111/j.1365-2966.2004.07765.x . arXiv:astro-ph/0311619 [astro-ph]

2004

Earlier work this paper cites.

Marsh TR, Nelemans G, Steeghs D (2004) Mass transfer between double white dwarfs. MNRAS 350(1):113–128. https://doi.org/10.1111/j.1365-2966.2004.07564.x . arXiv:astro-ph/0312577 [astro-ph]

2004

Earlier work this paper cites.

Matsubayashi T, Shinkai Ha, Ebisuzaki T (2004) Gravitational Waves from Merging Intermediate-Mass Black Holes. ApJ 614(2):864–868. https://doi.org/10.1086/423796

2004

Earlier work this paper cites.

Mayer L, Wadsley J (2004) The formation and evolution of bars in low surface brightness galaxies with cold dark matter haloes. MNRAS 347(1):277–294. https://doi.org/10.1111/j.1365-2966.2004.07202.x . arXiv:astro-ph/0303239 [astro-ph]

2004

Earlier work this paper cites.

Memmesheimer RM, Gopakumar A, Schäfer G (2004) Third post-Newtonian accurate generalized quasi-Keplerian parametrization for compact binaries in eccentric orbits. Phys. Rev. D 70(10):104011. https://doi.org/10.1103/PhysRevD.70.104011 . gr-qc/0407049

2004

Earlier work this paper cites.

Merritt D (2004) Evolution of the Dark Matter Distribution at the Galactic Center. Phys. Rev. Lett. 92(20):201304. https://doi.org/10.1103/PhysRevLett.92.201304 . arXiv:astro-ph/0311594 [astro-ph]

2004

Earlier work this paper cites.

Merritt D, Poon MY (2004) Chaotic Loss Cones and Black Hole Fueling. ApJ 606(2):788–798. https://doi.org/10.1086/382497 . arXiv:astro-ph/0302296 [astro-ph]

2004

Earlier work this paper cites.

Merritt D, Milosavljević M, Favata M, Hughes SA, Holz DE (2004) Consequences of Gravitational Radiation Recoil. ApJ 607(1):L9–L12. https://doi.org/10.1086/421551 . arXiv:astro-ph/0402057 [astro-ph]

2004

Earlier work this paper cites.

Miller MC, Colbert EJM (2004) Intermediate-Mass Black Holes. International Journal of Modern Physics D 13:1–64. https://doi.org/10.1142/S0218271804004426 . arXiv:astro-ph/0308402

2004

Earlier work this paper cites.

Misra D, Fragos T, Tauris TM, Zapartas E, Aguilera-Dena DR (2020) The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors. A&A 642:A174. https://doi.org/10.1051/0004-6361/202038070 . arXiv:2004.01205 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Nelemans G, Jonker PG, Marsh TR, van der Klis M (2004a) Optical spectra of the carbon-oxygen accretion discs in the ultra-compact X-ray binaries 4U 0614+09, 4U 1543-624 and 2S 0918-549. MNRAS 348(1):L7–L11. https://doi.org/10.1111/j.1365-2966.2004.07486.x . arXiv:astro-ph/0312008 [astro-ph]

2004

Earlier work this paper cites.

Nelemans G, Yungelson LR, Portegies Zwart SF (2004b) Short-period AM CVn systems as optical, X-ray and gravitational-wave sources. MNRAS 349(1):181–192. https://doi.org/10.1111/j.1365-2966.2004.07479.x . arXiv:astro-ph/0312193 [astro-ph]

2004

Earlier work this paper cites.

Ossokine S, Buonanno A, Marsat S, Cotesta R, Babak S, Dietrich T, Haas R, Hinder I, Pfeiffer HP, Pürrer M, et al. (2020) Multipolar effective-one-body waveforms for precessing binary black holes: Construction and validation. Phys. Rev. D 102(4):044055. https://doi.org/10.1103/PhysRevD.102.044055 . arXiv:2004.09442 [gr-qc]

Original

2004

Earlier work this paper cites.

Pacucci F, Loeb A (2020) Separating Accretion and Mergers in the Cosmic Growth of Black Holes with X-Ray and Gravitational-wave Observations. ApJ 895(2):95. https://doi.org/10.3847/1538-4357/ab886e . arXiv:2004.07246 [astro-ph.GA]

Original

2004

Earlier work this paper cites.

Pieroni M, Barausse E (2020) Foreground cleaning and template-free stochastic background extraction for LISA. J. Cosmology Astropart. Phys. 2020(7):021. https://doi.org/10.1088/1475-7516/2020/07/021 . arXiv:2004.01135 [astro-ph.CO]

Original

2004

Earlier work this paper cites.

Piovano GA, Maselli A, Pani P (2020) Extreme mass ratio inspirals with spinning secondary: A detailed study of equatorial circular motion. Phys. Rev. D 102(2):024041. https://doi.org/10.1103/PhysRevD.102.024041 . arXiv:2004.02654 [gr-qc]

Original

2004

Earlier work this paper cites.

Podsiadlowski P, Langer N, Poelarends AJT, Rappaport S, Heger A, Pfahl E (2004) The Effects of Binary Evolution on the Dynamics of Core Collapse and Neutron Star Kicks. ApJ 612(2):1044–1051. https://doi.org/10.1086/421713 . arXiv:astro-ph/0309588 [astro-ph]

2004

Earlier work this paper cites.

Portegies Zwart SF, Baumgardt H, Hut P, Makino J, McMillan SLW (2004) Formation of massive black holes through runaway collisions in dense young star clusters. Nature 428(6984):724–726. https://doi.org/10.1038/nature02448 . arXiv:astro-ph/0402622 [astro-ph]

2004

Earlier work this paper cites.

Reid MJ, Brunthaler A (2004) The Proper Motion of Sagittarius A*. II. The Mass of Sagittarius A*. ApJ 616(2):872–884. https://doi.org/10.1086/424960 . arXiv:astro-ph/0408107 [astro-ph]

2004

Earlier work this paper cites.

Santoliquido F, Mapelli M, Bouffanais Y, Giacobbo N, Di Carlo UN, Rastello S, Artale MC, Ballone A (2020a) The Cosmic Merger Rate Density Evolution of Compact Binaries Formed in Young Star Clusters and in Isolated Binaries. ApJ 898(2):152. https://doi.org/10.3847/1538-4357/ab9b78 . arXiv:2004.09533 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Secunda A, Bellovary J, Mac Low MM, Ford KES, McKernan B, Leigh NWC, Lyra W, Sándor Z, Adorno JI (2020a) Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes II. Spins and Incoming Objects. arXiv e-prints arXiv:2004.11936. arXiv:2004.11936 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Shemmer O, Netzer H, Maiolino R, Oliva E, Croom S, Corbett E, di Fabrizio L (2004) Near-Infrared Spectroscopy of High-Redshift Active Galactic Nuclei. I. A Metallicity-Accretion Rate Relationship. ApJ 614(2):547–557. https://doi.org/10.1086/423607 . arXiv:astro-ph/0406559 [astro-ph]

2004

Earlier work this paper cites.

Strohmayer TE (2004) Chandra Detection of the AM Canum Venaticorum Binary ES Ceti (KUV 01584-0939). ApJ 614(1):358–362. https://doi.org/10.1086/423615 . arXiv:astro-ph/0405203 [astro-ph]

2004

Earlier work this paper cites.

Tanaka H, Ward WR (2004) Three-dimensional Interaction between a Planet and an Isothermal Gaseous Disk. II. Eccentricity Waves and Bending Waves. ApJ 602(1):388–395. https://doi.org/10.1086/380992

2004

Earlier work this paper cites.

Toonen S, Portegies Zwart S, Hamers AS, Band opadhyay D (2020) The evolution of stellar triples. The most common evolutionary pathways. A&A 640:A16. https://doi.org/10.1051/0004-6361/201936835 . arXiv:2004.07848 [astro-ph.SR]

Original

2004

Earlier work this paper cites.

Toubiana A, Marsat S, Babak S, Barausse E, Baker J (2020a) Tests of general relativity with stellar-mass black hole binaries observed by LISA. Phys. Rev. D 101(10):104038. https://doi.org/10.1103/PhysRevD.101.104038 . arXiv:2004.03626 [gr-qc]

Original

2004

Earlier work this paper cites.

Whalen D, Abel T, Norman ML (2004) Radiation Hydrodynamic Evolution of Primordial H II Regions. ApJ 610(1):14–22. https://doi.org/10.1086/421548 . arXiv:astro-ph/0310283 [astro-ph]

2004

Earlier work this paper cites.

Zhu XJ, Thrane E (2020) Toward the Unambiguous Identification of Supermassive Binary Black Holes through Bayesian Inference. ApJ 900(2):117. https://doi.org/10.3847/1538-4357/abac5a . arXiv:2004.10944 [astro-ph.HE]

Original

2004

Earlier work this paper cites.

Anderson SF, Haggard D, Homer L, Joshi NR, Margon B, Silvestri NM, Szkody P, et al (2005) Ultracompact AM Canum Venaticorum Binaries from the Sloan Digital Sky Survey: Three Candidates Plus the First Confirmed Eclipsing System. AJ 130(5):2230–2236. https://doi.org/10.1086/491587 . arXiv:astro-ph/0506730 [astro-ph]

2005

Earlier work this paper cites.

Arzoumanian Z, Baker PT, Brazier A, Brook PR, Burke-Spolaor S, Bécsy B, Charisi M, Chatterjee S, Cordes JM, Cornish NJ, et al. (2020b) Multimessenger Gravitational-wave Searches with Pulsar Timing Arrays: Application to 3C 66B Using the NANOGrav 11-year Data Set. ApJ 900(2):102. https://doi.org/10.3847/1538-4357/ababa1 . arXiv:2005.07123 [astro-ph.GA]

Original

2005

Earlier work this paper cites.

Bender R, Kormendy J, Bower G, Green R, Thomas J, Danks AC, Gull T, Hutchings JB, Joseph CL, Kaiser ME, et al. (2005) HST STIS Spectroscopy of the Triple Nucleus of M31: Two Nested Disks in Keplerian Rotation around a Supermassive Black Hole. ApJ 631(1):280–300. https://doi.org/10.1086/432434 . arXiv:astro-ph/0509839 [astro-ph]

2005

Earlier work this paper cites.

Berczik P, Merritt D, Spurzem R (2005) Long-Term Evolution of Massive Black Hole Binaries. II. Binary Evolution in Low-Density Galaxies. ApJ 633(2):680–687. https://doi.org/10.1086/491598 . arXiv:astro-ph/0507260 [astro-ph]

2005

Earlier work this paper cites.

Bertone G, Merritt D (2005) Time-dependent models for dark matter at the galactic center. Phys. Rev. D 72(10):103502. https://doi.org/10.1103/PhysRevD.72.103502 . arXiv:astro-ph/0501555 [astro-ph]

2005

Earlier work this paper cites.

Bertone G, Zentner AR, Silk J (2005) New signature of dark matter annihilations: Gamma rays from intermediate-mass black holes. Phys. Rev. D 72(10):103517. https://doi.org/10.1103/PhysRevD.72.103517 . arXiv:astro-ph/0509565 [astro-ph]

2005

Earlier work this paper cites.

Blanchet L, Qusailah MSS, Will CM (2005) Gravitational Recoil of Inspiraling Black Hole Binaries to Second Post-Newtonian Order. ApJ 635(1):508–515. https://doi.org/10.1086/497332 . arXiv:astro-ph/0507692 [astro-ph]

2005

Earlier work this paper cites.

Bortolas E, Capelo PR, Zana T, Mayer L, Bonetti M, Dotti M, Davies MB, Madau P (2020) Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe. MNRAS 498(3):3601–3615. https://doi.org/10.1093/mnras/staa2628 . arXiv:2005.02409 [astro-ph.GA]

Original

2005

Earlier work this paper cites.

Chen Y, Yu Q, Lu Y (2020b) Dynamical Evolution of Cosmic Supermassive Binary Black Holes and Their Gravitational-wave Radiation. ApJ 897(1):86. https://doi.org/10.3847/1538-4357/ab9594 . arXiv:2005.10818 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Chicone C, Mashhoon B, Punsly B (2005) Relativistic motion of spinning particles in a gravitational field. Physics Letters A 343(1-3):1–7. https://doi.org/10.1016/j.physleta.2005.05.072 . arXiv:gr-qc/0504146 [gr-qc]

2005

Earlier work this paper cites.

Cornish NJ, Crowder J (2005) LISA data analysis using Markov chain Monte Carlo methods. Phys. Rev. D 72(4):043005. https://doi.org/10.1103/PhysRevD.72.043005 . arXiv:gr-qc/0506059 [astro-ph]

2005

Earlier work this paper cites.

Cornish NJ, Shuman K (2020) Black hole hunting with LISA. Phys. Rev. D 101(12):124008. https://doi.org/10.1103/PhysRevD.101.124008 . arXiv:2005.03610 [gr-qc]

Original

2005

Earlier work this paper cites.

Croton DJ, Springel V, White SDM, De Lucia G, Frenk CS, Gao L, Jenkins A, Kauffmann G, Navarro JF, Yoshida N (2006) The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies. MNRAS 365(1):11–28. https://doi.org/10.1111/j.1365-2966.2005.09675.x . arXiv:astro-ph/0508046 [astro-ph]

2005

Earlier work this paper cites.

Deme B, Hoang BM, Naoz S, Kocsis B (2020a) Detecting Kozai-Lidov Imprints on the Gravitational Waves of Intermediate-mass Black Holes in Galactic Nuclei. ApJ 901(2):125. https://doi.org/10.3847/1538-4357/abafa3 . arXiv:2005.03677 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Derdzinski A, D’Orazio D, Duffell P, Haiman Z, Macfadyen A (2020) Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band. arXiv e-prints arXiv:2005.11333. arXiv:2005.11333 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Dewi JDM, Podsiadlowski P, Pols OR (2005) The spin period-eccentricity relation of double neutron stars: evidence for weak supernova kicks? MNRAS 363(1):L71–L75. https://doi.org/10.1111/j.1745-3933.2005.00085.x . arXiv:astro-ph/0507628 [astro-ph]

2005

Earlier work this paper cites.

Di Matteo T, Springel V, Hernquist L (2005) Energy input from quasars regulates the growth and activity of black holes and their host galaxies. Nature 433(7026):604–607. https://doi.org/10.1038/nature03335 . arXiv:astro-ph/0502199 [astro-ph]

2005

Earlier work this paper cites.

Dieball A, Knigge C, Zurek DR, Shara MM, Long KS, Charles PA, Hannikainen DC, van Zyl L (2005) An Ultracompact X-Ray Binary in the Globular Cluster M15 (NGC 7078). ApJ 634(1):L105–L108. https://doi.org/10.1086/498712 . arXiv:astro-ph/0510430 [astro-ph]

2005

Earlier work this paper cites.

Dotti M, Colpi M, Haardt F (2006) Laser Interferometer Space Antenna double black holes: dynamics in gaseous nuclear discs. MNRAS 367(1):103–112. https://doi.org/10.1111/j.1365-2966.2005.09956.x . arXiv:astro-ph/0509813 [astro-ph]

2005

Earlier work this paper cites.

Edlund JA, Tinto M, Królak A, Nelemans G (2005) White-dwarf white-dwarf galactic background in the LISA data. Phys. Rev. D 71(12):122003. https://doi.org/10.1103/PhysRevD.71.122003 . arXiv:gr-qc/0504112 [gr-qc]

2005

Earlier work this paper cites.

Enoki M, Inoue KT, Nagashima M, Sugiyama N (2005) Gravitational waves from coalescing supermassive black hole binaries in a hierarchical galaxy formation model. Annual Report of the National Astronomical Observatory of Japan 7:34. arXiv:astro-ph/0502529 [astro-ph]

2005

Earlier work this paper cites.

Espaillat C, Patterson J, Warner B, Woudt P (2005) The Helium-rich Cataclysmic Variable ES Ceti. PASP 117(828):189–198. https://doi.org/10.1086/427959 . arXiv:astro-ph/0412068 [astro-ph]

2005

Earlier work this paper cites.

Farihi J, Becklin EE, Zuckerman B (2005) Low-Luminosity Companions to White Dwarfs. ApJS 161(2):394–428. https://doi.org/10.1086/444362 . arXiv:astro-ph/0506017 [astro-ph]

2005

Earlier work this paper cites.

Gilli R, Daddi E, Zamorani G, Tozzi P, Borgani S, Bergeron J, Giacconi R, Hasinger G, Mainieri V, Norman C, et al. (2005) The spatial clustering of X-ray selected AGN and galaxies in the Chandra Deep Field South and North. A&A 430:811–825. https://doi.org/10.1051/0004-6361:20041375 . arXiv:astro-ph/0409759 [astro-ph]

2005

Earlier work this paper cites.

Hamers AS, Safarzadeh M (2020) Was GW190412 Born from a Hierarchical 3 + 1 Quadruple Configuration? ApJ 898(2):99. https://doi.org/10.3847/1538-4357/ab9b27 . arXiv:2005.03045 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Hobbs G, Lorimer DR, Lyne AG, Kramer M (2005) A statistical study of 233 pulsar proper motions. MNRAS 360(3):974–992. https://doi.org/10.1111/j.1365-2966.2005.09087.x . arXiv:astro-ph/0504584 [astro-ph]

2005

Earlier work this paper cites.

Huang SJ, Hu YM, Korol V, Li PC, Liang ZC, Lu Y, Wang HT, Yu S, Mei J (2020) Science with the TianQin Observatory: Preliminary results on Galactic double white dwarf binaries. arXiv e-prints arXiv:2005.07889. arXiv:2005.07889 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

in’t Zand JJM, Cumming A, van der Sluys MV, Verbunt F, Pols OR (2005) On the possibility of a helium white dwarf donor in the presumed ultracompact binary 2S 0918-549. A&A 441(2):675–684. https://doi.org/10.1051/0004-6361:20053002 . arXiv:astro-ph/0506666 [astro-ph]

2005

Earlier work this paper cites.

Kimpson T, Wu K, Zane S (2020a) Gravitational burst radiation from pulsars in the Galactic centre and stellar clusters. MNRAS 495(1):600–613. https://doi.org/10.1093/mnras/staa1259 . arXiv:2005.02053 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Lenon AK, Nitz AH, Brown DA (2020) Measuring the eccentricity of GW170817 and GW190425. MNRAS 497(2):1966–1971. https://doi.org/10.1093/mnras/staa2120 . arXiv:2005.14146 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Merritt D, Milosavljević M (2005) Massive Black Hole Binary Evolution. Living Reviews in Relativity 8:8. https://doi.org/10.12942/lrr-2005-8 . arXiv:astro-ph/0410364 [astro-ph]

2005

Earlier work this paper cites.

Miller MC (2005) Probing General Relativity with Mergers of Supermassive and Intermediate-Mass Black Holes. ApJ 618(1):426–431. https://doi.org/10.1086/425910 . arXiv:astro-ph/0409331 [astro-ph]

2005

Earlier work this paper cites.

Miller MC, Freitag M, Hamilton DP, Lauburg VM (2005) Binary Encounters with Supermassive Black Holes: Zero-Eccentricity LISA Events. ApJ 631(2):L117–L120. https://doi.org/10.1086/497335 . arXiv:astro-ph/0507133 [astro-ph]

2005

Earlier work this paper cites.

Milosavljević M, Phinney ES (2005) The Afterglow of Massive Black Hole Coalescence. ApJ 622(2):L93–L96. https://doi.org/10.1086/429618 . arXiv:astro-ph/0410343 [astro-ph]

2005

Earlier work this paper cites.

Miralda-Escudé J, Kollmeier JA (2005) Star Captures by Quasar Accretion Disks: A Possible Explanation of the M- σ \sigma Relation. ApJ 619(1):30–40. https://doi.org/10.1086/426467 . arXiv:astro-ph/0310717 [astro-ph]

2005

Earlier work this paper cites.

Murguia-Berthier A, Batta A, Janiuk A, Ramirez-Ruiz E, Mandel I, Noble SC, Everson RW (2020) On the Maximum Stellar Rotation to form a Black Hole without an Accompanying Luminous Transient. ApJ 901(2):L24. https://doi.org/10.3847/2041-8213/abb818 . arXiv:2005.10212 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Nelemans G, Napiwotzki R, Karl C, Marsh TR, Voss B, Roelofs G, Izzard RG, Montgomery M, Reerink T, Christlieb N, et al. (2005) Binaries discovered by the SPYproject. IV. Five single-lined DA double white dwarfs. A&A 440(3):1087–1095. https://doi.org/10.1051/0004-6361:20053174 . arXiv:astro-ph/0506231 [astro-ph]

2005

Earlier work this paper cites.

Pretorius F (2005) Evolution of Binary Black-Hole Spacetimes. Phys. Rev. Lett. 95(12):121101. https://doi.org/10.1103/PhysRevLett.95.121101 . arXiv:gr-qc/0507014 [gr-qc]

2005

Earlier work this paper cites.

Ramsay G, Hakala P (2005) RApid Temporal Survey (RATS) - I. Overview and first results. MNRAS 360(1):314–321. https://doi.org/10.1111/j.1365-2966.2005.09035.x . arXiv:astro-ph/0503138 [astro-ph]

2005

Earlier work this paper cites.

Ramsay G, Hakala P, Marsh T, Nelemans G, Steeghs D, Cropper M (2005) XMM-Newton observations of AM CVn binaries. A&A 440(2):675–681. https://doi.org/10.1051/0004-6361:20052950 . arXiv:astro-ph/0505549 [astro-ph]

2005

Earlier work this paper cites.

Rossi EM, Stone NC, Law-Smith JAP, MacLeod M, Lodato G, Dai JL, Mand el I (2020) The Process of Stellar Tidal Disruption by Supermassive Black Holes. The first pericenter passage. arXiv e-prints arXiv:2005.12528. arXiv:2005.12528 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Sesana A, Haardt F, Madau P, Volonteri M (2005) The Gravitational Wave Signal from Massive Black Hole Binaries and Its Contribution to the LISA Data Stream. ApJ 623(1):23–30. https://doi.org/10.1086/428492 . arXiv:astro-ph/0409255 [astro-ph]

2005

Earlier work this paper cites.

Springel V, Di Matteo T, Hernquist L (2005b) Modelling feedback from stars and black holes in galaxy mergers. MNRAS 361(3):776–794. https://doi.org/10.1111/j.1365-2966.2005.09238.x . arXiv:astro-ph/0411108 [astro-ph]

2005

Earlier work this paper cites.

Stritzinger MD, Taddia F, Fraser M, Tauris TM, Contreras C, Drybye S, Galbany L, Holmbo S, Morrell N, Pastorello A, et al. (2020) The Carnegie Supernova Project II. Observations of the luminous red nova AT 2014ej. A&A 639:A104. https://doi.org/10.1051/0004-6361/202038019 . arXiv:2005.00076 [astro-ph.HE]

Original

2005

Earlier work this paper cites.

Strohmayer TE (2005) Precision X-Ray Timing of RX J0806.3+1527 with Chandra: Evidence for Gravitational Radiation from an Ultracompact Binary. ApJ 627(2):920–925. https://doi.org/10.1086/430439 . arXiv:astro-ph/0504150 [astro-ph]

2005

Earlier work this paper cites.

Thompson TA, Quataert E, Murray N (2005) Radiation Pressure–supported Starburst Disks and Active Galactic Nucleus Fueling. ApJ 630(1):167–185. https://doi.org/10.1086/431923 , URL http://dx.doi.org/10.1086/431923

2005

Earlier work this paper cites.

Tiede C, Zrake J, MacFadyen A, Haiman Z (2020) Gas-driven inspiral of binaries in thin accretion disks. arXiv e-prints arXiv:2005.09555. arXiv:2005.09555 [astro-ph.GA]

Original

2005

Earlier work this paper cites.

Umstätter R, Christensen N, Hendry M, Meyer R, Simha V, Veitch J, Vigeland S, Woan G (2005) Bayesian modeling of source confusion in LISA data. Phys. Rev. D 72(2):022001. https://doi.org/10.1103/PhysRevD.72.022001 . arXiv:gr-qc/0506055 [gr-qc]

2005

Earlier work this paper cites.

van den Heuvel EPJ, Tauris TM (2020) Comment on “A noninteracting low-mass black hole-giant star binary system”. Science 368(6491):eaba3282. https://doi.org/10.1126/science.aba3282 . arXiv:2005.04896 [astro-ph.SR]

Original

2005

Earlier work this paper cites.

van der Sluys MV, Verbunt F, Pols OR (2005) Reduced magnetic braking and the magnetic capture model for the formation of ultra-compact binaries. A&A 440(3):973–979. https://doi.org/10.1051/0004-6361:20052696 . arXiv:astro-ph/0506375 [astro-ph]

2005

Cited alongside, same era.

Volonteri M, Perna R (2005) Dynamical evolution of intermediate-mass black holes and their observable signatures in the nearby Universe. MNRAS 358(3):913–922. https://doi.org/10.1111/j.1365-2966.2005.08832.x . arXiv:astro-ph/0501345 [astro-ph]

2005

Cited alongside, same era.

Volonteri M, Madau P, Quataert E, Rees MJ (2005) The Distribution and Cosmic Evolution of Massive Black Hole Spins. ApJ 620(1):69–77. https://doi.org/10.1086/426858 . arXiv:astro-ph/0410342 [astro-ph]

2005

Cited alongside, same era.

Volonteri M, Pfister H, Beckmann RS, Dubois Y, Colpi M, Conselice CJ, Dotti M, Martin G, Jackson R, Kraljic K, et al. (2020) Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations. MNRAS 498:2219. https://doi.org/10.1093/mnras/staa2384 . arXiv:2005.04902 [astro-ph.GA]

Original

van Oirschot P, Nelemans G, Toonen S, Pols O, Brown AGA, Helmi A, Portegies Zwart S (2014) Binary white dwarfs in the halo of the Milky Way. A&A 569:A42. https://doi.org/10.1051/0004-6361/201424195 . arXiv:1407.2405 [astro-ph.GA]

Original

2014

Later among the works it cites.

Van Wassenhove S, Capelo PR, Volonteri M, Dotti M, Bellovary JM, Mayer L, Governato F (2014) Nuclear coups: dynamics of black holes in galaxy mergers. MNRAS 439(1):474–487. https://doi.org/10.1093/mnras/stu024 . arXiv:1310.7581 [astro-ph.CO]

Original

2014

Later among the works it cites.

Visbal E, Haiman Z, Bryan GL (2014) Direct collapse black hole formation from synchronized pairs of atomic cooling haloes. MNRAS 445(1):1056–1063. https://doi.org/10.1093/mnras/stu1794 . arXiv:1406.7020 [astro-ph.GA]

Original

2014

Later among the works it cites.

Vogelsberger M, Genel S, Springel V, Torrey P, Sijacki D, Xu D, Snyder G, Nelson D, Hernquist L (2014) Introducing the Illustris Project: simulating the coevolution of dark and visible matter in the Universe. MNRAS 444(2):1518–1547. https://doi.org/10.1093/mnras/stu1536 . arXiv:1405.2921 [astro-ph.CO]

Original