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1910
Earlier work this paper cites.
Boesgaard, A. M. & M. J. Tripicco, Lithium in the Hyades Cluster , ApJ, 302
1986
Earlier work this paper cites.
Boesgaard, A. M., C. P. Deliyannis, A. Stephens, & D. L. Lambert, Boron in Lithium- and Beryllium-deficient F Stars , ApJ, 492
1998
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C. Allende Prieto, M. Aplund,G., R.J. García López,Signature of convection in the spectrum of Procyon: fundamental parameters and iron abundance, Astrophys.J. 567, 544 (2002)
2002
Earlier work this paper cites.
Jedamzik, K., Neutralinos, big bang nucleosynthesis, and 6 Li in low-metallicity stars , PhRvD, 70
2004
Earlier work this paper cites.
Wedemeyer, S., B. Freytag, M. Steffen, H.-G. Ludwig, & H. Holweger, Numerical simulation of the 3D structure and dynamics of the non-magnetic solar chromosphere , A&A, 414
2004
Earlier work this paper cites.
Charbonnel, C. & F. Primas, The lithium content of the Galactic Halo stars , A&A, 442
2005
Earlier work this paper cites.
Alecian, G., O. Richard, & S. Vauclair, Element stratification in stars : 40 years of atomic diffusion; Meeting in Honour of Georges Michaud , EAS, 17
2005
Earlier work this paper cites.
Piau, L., T. C. Beers, D. S. Balsara, T. Sivarani, J. W. Truran, & J. W. Ferguson, From First Stars to the Spite Plateau: A Possible Reconciliation of Halo Stars Observations with Predictions from Big Bang Nucleosynthesis , ApJ, 653
2006
Earlier work this paper cites.
N., Prantzos Early galactic chemical evolution , Proceedings of the International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos - IX. 25-30 June 2006, CERN, PoS p.254 , (2006)
2006
Cited alongside, same era.
Asplund, M., D. L. Lambert, P. E. Nissen, F. Primas, & V. V. Smith, Lithium Isotopic Abundances in Metal-poor Halo Stars , ApJ, 644
2006
Cited alongside, same era.
Rollinde, E., E. Vangioni, & K. A. Olive, Population III Generated Cosmic Rays and the Production of 6 Li , ApJ, 651
2006
Cited alongside, same era.
Prantzos, N., The energetics, evolution, and stellar depletion of 6 Li in the early Galaxy , A&A, 448
2006
Cited alongside, same era.
Spergel, D. N., R. Bean, O. Doré, et al., Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology , ApJS, 170
2007
Cited alongside, same era.
Bonifacio, P., P. Molaro, T. Sivarani, et al., First stars VII - Lithium in extremely metal poor dwarfs , A&A, 462
2007
Later among the works it cites.
Cayrel, R., M. Steffen, H. Chand, et al., Line shift, line asymmetry, and the Li 6 / 7 Li \rm{}^{6}Li/^{7}Li isotopic ratio determination , A&A, 473
2007
Later among the works it cites.
Jedamzik, K., Cosmic Li6 and Li7 problems and BBN with long-lived charged massive particles , PhRvD, 77
2008
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Charbonnel, C. & S. Talon, Deep inside low-mass stars , IAUS, 252
2008
Closest in time.
González Hernández, J. I., P. Bonifacio, H.-G. Ludwig, et al., First stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876-032 , A&A, 480
2008
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2007
Cited alongside, same era.
Cumberbatch, D., K. Ichikawa, M. Kawasaki, K. Kohri, J. Silk, & G. D. Starkman, Solving the cosmic lithium problems with primordial late-decaying particles , PhRvD, 76
2007
Cited alongside, same era.
Kusakabe, M., T. Kajino, R. N. Boyd, T. Yoshida, & G. J. Mathews, Simultaneous solution to the Li6 and Li7 big bang nucleosynthesis problems from a long-lived negatively charged leptonic particle , PhRvD, 76
2007
Cited alongside, same era.
Korn, A. J., F. Grundahl, O. Richard, L. Mashonkina, P. S. Barklem, R. Collet, B. Gustafsson, & N. Piskunov, Atomic Diffusion and Mixing in Old Stars. I. Very Large Telescope FLAMES-UVES Observations of Stars in NGC 6397 , ApJ, 671
2007
Cited alongside, same era.
Garcia Perez, A.E. Poster at this meeting (2008)
2008
Closest in time.
Frebel, A., R. Collet, K. Eriksson, N. Christlieb, & W. Aoki, HE 1327-2326, an Unevolved Star with [Fe/H] < − 5.0 <-5.0 . II. New 3D-1D Corrected Abundances from a Very Large Telescope UVES Spectrum , ApJ, 684
2008
Closest in time.
Evoli, C., S. Salvadori, & A. Ferrara, The puzzling origin of the 6 Li plateau , MNRAS, 390
2008
Closest in time.