Adams, Fred C.; Laughlin, Gregory. A Dying Universe: The Long Term Fate and Evolution of Astrophysical Objects. Reviews of Modern Physics. April 1997, 69 (2): 337–372. Bibcode:1997RvMP...69..337A. doi:10.1103/RevModPhys.69.337.
Luck, R. Earle; Heiter, Ulrike. Stars within 15 Parsecs: Abundances for a Northern Sample. The Astronomical Journal. 2005, 129 (2): 1063–1083. Bibcode:2005AJ....129.1063L. doi:10.1086/427250.
Bahcall, John N.; Pinsonneault, M. H.; Basu, Sarbani. Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties. The Astrophysical Journal. 2001-07-10, 555 (2): 990–1012. Bibcode:2003PhRvL..90m1301B. doi:10.1086/321493.
Oey, M. S.; Clarke, C. J. Statistical Confirmation of a Stellar Upper Mass Limit. The Astrophysical Journal. 2005, 620 (1): L43–L46. Bibcode:2005ApJ...620L..43O. doi:10.1086/428396.引文使用过时参数coauthors (帮助)
Burrows, A.; Hubbard, W. B.; Saumon, D.; Lunine, J. I. An expanded set of brown dwarf and very low mass star models. Astrophysical Journal, Part 1. March 1993, 406 (1): 158–171. Bibcode:1993ApJ...406..158B. doi:10.1086/172427.
Fynbo, Hans O. U.; et al. Revised rates for the stellar triple-α process from measurement of 12C nuclear resonances. Nature. 2004, 433 (7022): 136–139. PMID 15650733. doi:10.1038/nature03219. 引文格式1维护:显式使用等标签 (link)
Girardi, L.; Bressan, A.; Bertelli, G.; Chiosi, C. Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 Msun, and from Z=0.0004 to 0.03. Astronomy and Astrophysics Supplement. 2000, 141 (3): 371–383. doi:10.1051/aas:2000126.
Adams, Fred C.; Laughlin, Gregory. A Dying Universe: The Long Term Fate and Evolution of Astrophysical Objects. Reviews of Modern Physics. April 1997, 69 (2): 337–372. Bibcode:1997RvMP...69..337A. doi:10.1103/RevModPhys.69.337.
Strömgren, Bengt. On the Interpretation of the Hertzsprung-Russell-Diagram. Zeitschrift für Astrophysik. 1933, 7: 222–248. Bibcode:1933ZA......7..222S.
Luck, R. Earle; Heiter, Ulrike. Stars within 15 Parsecs: Abundances for a Northern Sample. The Astronomical Journal. 2005, 129 (2): 1063–1083. Bibcode:2005AJ....129.1063L. doi:10.1086/427250.
Bahcall, John N.; Pinsonneault, M. H.; Basu, Sarbani. Solar Models: Current Epoch and Time Dependences, Neutrinos, and Helioseismological Properties. The Astrophysical Journal. 2001-07-10, 555 (2): 990–1012. Bibcode:2003PhRvL..90m1301B. doi:10.1086/321493.
Oey, M. S.; Clarke, C. J. Statistical Confirmation of a Stellar Upper Mass Limit. The Astrophysical Journal. 2005, 620 (1): L43–L46. Bibcode:2005ApJ...620L..43O. doi:10.1086/428396.引文使用过时参数coauthors (帮助)
Burrows, A.; Hubbard, W. B.; Saumon, D.; Lunine, J. I. An expanded set of brown dwarf and very low mass star models. Astrophysical Journal, Part 1. March 1993, 406 (1): 158–171. Bibcode:1993ApJ...406..158B. doi:10.1086/172427.
Bressan, A. G.; Chiosi, C.; Bertelli, G. Mass loss and overshooting in massive stars. Astronomy and Astrophysics. 1981, 102 (1): 25–30. Bibcode:1981A&A...102...25B.
Burgasser, Adam J.; Kirkpatrick, J. Davy; Lepine, Sebastien. Spitzer Studies of Ultracool Subdwarfs: Metal-poor Late-type M, L and T Dwarfs. Proceedings of the 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun. Hamburg, Germany: Dordrecht, D. Reidel Publishing Co: 237. July 5–9, 2004 [2007-12-06].引文使用过时参数coauthors (帮助)
Fynbo, Hans O. U.; et al. Revised rates for the stellar triple-α process from measurement of 12C nuclear resonances. Nature. 2004, 433 (7022): 136–139. PMID 15650733. doi:10.1038/nature03219. 引文格式1维护:显式使用等标签 (link)
Harding E. Smith. The Hertzsprung-Russell Diagram. Gene Smith's Astronomy Tutorial. Center for Astrophysics & Space Sciences, University of California, San Diego. 1999-04-21 [2009-10-29]. (原始内容存档于2010-06-17).
Siess, Lionel. Computation of Isochrones. Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles. 2000 [2007-12-06].[永久失效連結]—Compare, for example, the model isochrones generated for a ZAMS of 1.1 solar masses. This is listed in the table as 1.26 times the solar luminosity. At metallicity Z=0.01 the luminosity is 1.34 times solar luminosity. At metallicity Z=0.04 the luminosity is 0.89 times the solar luminosity.
Harding E. Smith. The Hertzsprung-Russell Diagram. Gene Smith's Astronomy Tutorial. Center for Astrophysics & Space Sciences, University of California, San Diego. 1999-04-21 [2009-10-29]. (原始内容存档于2010-06-17).