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Type Ia supernovae (SNe) serve as a fundamental pillar of modern cosmology, owing to their large luminosity and a well-defined relationship between light-curve shape and peak brightness.
Binaries and Supernovae of Type I
Whelan, J. & Iben, I., Jr · 1973
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Accreting white dwarf models for type I supernovae. I - Presupernova evolution and triggering mechanisms
Nomoto, K · 1982
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Supernovae of type I as end products of the evolution of binaries with components of moderate initial mass (M not greater than about 9 solar masses)
Iben, I., Jr. & Tutukov, A. V · 1984
Earlier work this paper cites.
Double white dwarfs as progenitors of R Coronae Borealis stars and Type I supernovae
Webbink, R. F · 1984
Earlier work this paper cites.
Are symbiotic stars the precursors of type IA supernovae?
Munari, U. & Renzini, A · 1992
Earlier work this paper cites.
Accreting white dwarf models for CAL 83, CAL 87 and other ultrasoft X-ray sources in the LMC
van den Heuvel, E. P. J., Bhattacharya, D., Nomoto, K. & Rappaport, S. A · 1992
Earlier work this paper cites.
The absolute magnitudes of Type IA supernovae
Phillips, M. M · 1993
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Optical Spectra of Supernovae
Filippenko, A. V · 1997
Earlier work this paper cites.
Type Ia supernovae: their origin and possible applications in cosmology
Nomoto, K., Iwamoto, K. & Kishimoto, N · 1997
Earlier work this paper cites.
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
Riess, A. G. et al · 1998
Earlier work this paper cites.
The Extragalactic Distance Scale Key Project. XVI. Cepheid Variables in an Inner Field of M101
Stetson, P. B. et al · 1998
Cited alongside, same era.
Measurements of Omega and Lambda from 42 High-Redshift Supernovae
Perlmutter, S. et al · 1999
Cited alongside, same era.
A New Evolutionary Path to Type IA Supernovae: A Helium-rich Supersoft X-Ray Source Channel
Hachisu, I., Kato, M., Nomoto, K. & Umeda, H · 1999
Cited alongside, same era.
Catalog of supersoft X-ray sources
Greiner, J · 2000
Cited alongside, same era.
Recurrent Novae as a Progenitor System of Type Ia Supernovae. I. RS Ophiuchi Subclass: Systems with a Red Giant Companion
Hachisu, I. & Kato, M · 2001
Cited alongside, same era.
The mass of the white dwarf in the recurrent nova U Scorpii
Thoroughgood, T. D., Dhillon, V. S., Littlefair, S. P., Marsh, T. R. & Smith, D. A · 2001
Helium Nova on a Very Massive White Dwarf: A Revised Light-Curve Model of V445 Puppis (2000)
Kato, M., Hachisu, I., Kiyota, S. & Saio, H · 2008
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Helium-star evolutionary channel to super-Chandrasekhar mass type Ia supernovae
Liu, W.-M., Chen, W.-C., Wang, B. & Han, Z. W · 2010
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Comprehensive Photometric Histories of All Known Galactic Recurrent Novae
Schaefer, B. E · 2010
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The Progenitors of Type Ia Supernovae. I. Are they Supersoft Sources?
Di Stefano, R · 2010
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The Progenitors of Type Ia Supernovae. II. Are they Double-degenerate Binaries? The Symbiotic Channel
Di Stefano, R · 2010
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On the Use of Empirical Bolometric Corrections for Stars
Torres, G · 2010
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Cited alongside, same era.
The W. M. Keck Observatory Laser Guide Star Adaptive Optics System: Overview
Wizinowich, P. L. et al · 2006
Cited alongside, same era.
A Common Explosion Mechanism for Type Ia Supernovae
Mazzali, P. A., Röpke, F. K., Benetti, S. & Hillebrandt, W · 2007
Cited alongside, same era.
Remnant evolution after a carbon-oxygen white dwarf merger
Yoon, S.-C., Podsiadlowski, P. & Rosswog, S · 2007
Cited alongside, same era.
The nuclear diversity of Type Ia supernova explosions
Podsiadlowski, P., Mazzali, P., Lesaffre, P., Han, Z. & Förster, F · 2008
Cited alongside, same era.
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Type Ia supernovae as stellar endpoints and cosmological tools
Howell, D. A · 2011
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A New Cepheid Distance to the Giant Spiral M101 Based on Image Subtraction of Hubble Space Telescope/Advanced Camera for Surveys Observations
Shappee, B. J. & Stanek, K. Z · 2011
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Discovery of a Type Ia Supernova Within Hours of Explosion in the Pinwheel Galaxy (2011)
Nugent, P. et al · 2011
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The Long-Term Evolution of Double White Dwarf Mergers
Shen, K. J., Bildsten, L., Kasen, D. & Quataert, E · 2011
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