主序星 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "主序星" in Chinese language version.

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amazon.de

For a detailed historical reconstruction of the theoretical derivation of this relationship by Eddington in 1924, see: Lecchini, Stefano. How Dwarfs Became Giants. The Discovery of the Mass-Luminosity Relation. Bern Studies in the History and Philosophy of Science. 2007 [2011-04-15]. ISBN 3-9522882-6-8. （原始内容存档于2022-11-09）.

archive.org

Longair, Malcolm S. The Cosmic Century: A History of Astrophysics and Cosmology. Cambridge University Press. 2006: 25–26. ISBN 0-521-47436-1.
Brown, Laurie M.; Pais, Abraham; Pippard, A. B. (编). Twentieth Century Physics. Bristol; New York: Institute of Physics, American Institute of Physics. 1995: 1696. ISBN 0-7503-0310-7. OCLC 33102501.
Schatzman, Evry L.; Praderie, Francoise. The Stars. Springer. 1993: 96–97. ISBN 3-540-54196-9.
Gloeckler, George; Geiss, Johannes. Composition of the local interstellar medium as diagnosed with pickup ions. Advances in Space Research. 2004, 34 (1): 53–60. Bibcode:2004AdSpR..34...53G. doi:10.1016/j.asr.2003.02.054.
Clayton, Donald D. Principles of Stellar Evolution and Nucleosynthesis. University of Chicago Press. 1983. ISBN 0-226-10953-4.
Karttunen, Hannu. Fundamental Astronomy. Springer. 2003. ISBN 3-540-00179-4.
Salaris, Maurizio; Cassisi, Santi. Evolution of Stars and Stellar Populations. John Wiley and Sons. 2005: 128. ISBN 0-470-09220-3.
Ziebarth, Kenneth. On the Upper Mass Limit for Main-Sequence Stars. Astrophysical Journal. 1970, 162: 947–962. Bibcode:1970ApJ...162..947Z. doi:10.1086/150726.
Aller, Lawrence H. Atoms, Stars, and Nebulae. Cambridge University Press. 1991. ISBN 0-521-31040-7.
Tayler, Roger John. The Stars: Their Structure and Evolution. Cambridge University Press. 1994. ISBN 0-521-45885-4.
Sweet, I. P. A.; Roy, A. E. The structure of rotating stars. Monthly Notices of the Royal Astronomical Society. 1953, 113: 701–715. Bibcode:1953MNRAS.113..701S.
Arnett, David. Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present. Princeton University Press. 1996. ISBN 0-691-01147-8. —Hydrogen fusion produces 8×10¹⁸ erg/g while helium fusion produces 8×10¹⁷ erg/g.
Rolfs, Claus E.; Rodney, William S. Cauldrons in the Cosmos: Nuclear Astrophysics. University of Chicago Press. 1988. ISBN 0-226-72457-3.
Hansen, Carl J.; Kawaler, Steven D. Stellar Interiors: Physical Principles, Structure, and Evolution. Birkhäuser. 1994: 28. ISBN 0-387-94138-X.

astrophysicsspectator.com

Brainerd, Jerome James. Main-Sequence Stars. The Astrophysics Spectator. 2005-02-16 [2007-12-04]. （原始内容存档于2016-06-14）.

atlasoftheuniverse.com

Richard Powell. The Hertzsprung Russell Diagram. An Atlas of the Universe. 2006 [2009-10-29]. （原始内容存档于2010-12-31）.

caltech.edu

nedipac.caltech.edu

Morgan, W. W.; Keenan, P. C.; Kellman, E. An atlas of stellar spectra, with an outline of spectral classification. Chicago, Illinois: The University of Chicago press. 1943 [2008-08-12]. （原始内容存档于2011-05-14）.

csiro.au

outreach.atnf.csiro.au

Main Sequence Stars. Australia Telescope Outreach and Education. [2007-12-04]. （原始内容存档于2013-12-29）.
Staff. Post-Main Sequence Stars. Australia Telescope Outreach and Education. 2006-10-12 [2008-01-08]. （原始内容存档于2013-01-20）.

doi.org

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.
Gilmore, Gerry. The Short Spectacular Life of a Superstar. Science. 2004, 304 (5697): 1915–1916 [2007-05-01]. PMID 15218132. doi:10.1126/science.1100370. （原始内容存档于2009-02-01）.
Gloeckler, George; Geiss, Johannes. Composition of the local interstellar medium as diagnosed with pickup ions. Advances in Space Research. 2004, 34 (1): 53–60. Bibcode:2004AdSpR..34...53G. doi:10.1016/j.asr.2003.02.054.
Kroupa, Pavel. The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems. Science. 2002, 295 (5552): 82–91 [2007-12-03]. PMID 11778039. doi:10.1126/science.1067524. （原始内容存档于2009-11-25）.
Schilling, Govert. New Model Shows Sun Was a Hot Young Star. Science. 2001, 293 (5538): 2188–2189 [2007-02-04]. PMID 11567116. doi:10.1126/science.293.5538.2188. （原始内容存档于2009-01-31）.
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.
Ziebarth, Kenneth. On the Upper Mass Limit for Main-Sequence Stars. Astrophysical Journal. 1970, 162: 947–962. Bibcode:1970ApJ...162..947Z. doi:10.1086/150726.
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.
Gough, D. O. Solar interior structure and luminosity variations. Solar Physics. 1981, 74 (1): 21–34. Bibcode:1981SoPh...74...21G. doi:10.1007/BF00151270.
Wright, J. T. Do We Know of Any Maunder Minimum Stars?. The Astronomical Journal. 2004, 128 (3): 1273–1278 [2007-12-06]. doi:10.1086/423221.
Schröder, K.-P.; Connon Smith, Robert. Distant future of the Sun and Earth revisited. Monthly Notices of the Royal Astronomical Society. May 2008, 386 (1): 155–163. Bibcode:2008MNRAS.386..155S. doi:10.1111/j.1365-2966.2008.13022.x.
Sackmann, I.-Juliana; Boothroyd, Arnold I.; Kraemer, Kathleen E. Our Sun. III. Present and Future. Astrophysical Journal. November 1993, 418: 457–468. Bibcode:1993ApJ...418..457S. doi:10.1086/173407.
Laughlin, Gregory; Bodenheimer, Peter; Adams, Fred C. The End of the Main Sequence. The Astrophysical Journal. 1997, 482 (1): 420–432. Bibcode:1997ApJ...482..420L. doi:10.1086/304125.
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.
Girardi, L.; Bressan, A.; Bertelli, G.; Chiosi, C. Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 M_sun, and from Z=0.0004 to 0.03. Astronomy and Astrophysics Supplement. 2000, 141 (3): 371–383. doi:10.1051/aas:2000126.
Poelarends, A. J. T.; Herwig, F.; Langer, N.; Heger, A. The Supernova Channel of Super-AGB Stars. The Astrophysical Journal. March 2008, 675 (1): 614–625. doi:10.1086/520872.
Krauss, Lawrence M.; Chaboyer, Brian. Age Estimates of Globular Clusters in the Milky Way: Constraints on Cosmology. Science. 2003, 299 (5603): 65–69. PMID 12511641. doi:10.1126/science.1075631.

gsu.edu

chara.gsu.edu

Staff. List of the Nearest Hundred Nearest Star Systems. Research Consortium on Nearby Stars. 2008-01-01 [2008-08-12]. （原始内容存档于2012-05-13）.

harvard.edu

ui.adsabs.harvard.edu

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.
Russell, H. N. "Giant" and "dwarf" stars. The Observatory. 1913, 36: 324–329. Bibcode:1913Obs....36..324R.
Strömgren, Bengt. On the Interpretation of the Hertzsprung-Russell-Diagram. Zeitschrift für Astrophysik. 1933, 7: 222–248. Bibcode:1933ZA......7..222S.
Gloeckler, George; Geiss, Johannes. Composition of the local interstellar medium as diagnosed with pickup ions. Advances in Space Research. 2004, 34 (1): 53–60. Bibcode:2004AdSpR..34...53G. doi:10.1016/j.asr.2003.02.054.
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.
Ziebarth, Kenneth. On the Upper Mass Limit for Main-Sequence Stars. Astrophysical Journal. 1970, 162: 947–962. Bibcode:1970ApJ...162..947Z. doi:10.1086/150726.
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.
Gough, D. O. Solar interior structure and luminosity variations. Solar Physics. 1981, 74 (1): 21–34. Bibcode:1981SoPh...74...21G. doi:10.1007/BF00151270.
Sweet, I. P. A.; Roy, A. E. The structure of rotating stars. Monthly Notices of the Royal Astronomical Society. 1953, 113: 701–715. Bibcode:1953MNRAS.113..701S.
Schröder, K.-P.; Connon Smith, Robert. Distant future of the Sun and Earth revisited. Monthly Notices of the Royal Astronomical Society. May 2008, 386 (1): 155–163. Bibcode:2008MNRAS.386..155S. doi:10.1111/j.1365-2966.2008.13022.x.
Sackmann, I.-Juliana; Boothroyd, Arnold I.; Kraemer, Kathleen E. Our Sun. III. Present and Future. Astrophysical Journal. November 1993, 418: 457–468. Bibcode:1993ApJ...418..457S. doi:10.1086/173407.
Laughlin, Gregory; Bodenheimer, Peter; Adams, Fred C. The End of the Main Sequence. The Astrophysical Journal. 1997, 482 (1): 420–432. Bibcode:1997ApJ...482..420L. doi:10.1086/304125.

adsabs.harvard.edu

Wright, J. T. Do We Know of Any Maunder Minimum Stars?. The Astronomical Journal. 2004, 128 (3): 1273–1278 [2007-12-06]. doi:10.1086/423221.
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].

ads.harvard.edu

Zombeck, Martin V. Handbook of Space Astronomy and Astrophysics 2nd. Cambridge University Press. 1990 [2007-12-06]. ISBN 0-521-34787-4. （原始内容存档于2010-12-29）.

nasa.gov

imagine.gsfc.nasa.gov

Lochner, Jim; Gibb, Meredith; Newman, Phil. Stars. NASA. 2006-09-06 [2007-12-05]. （原始内容存档于2014-11-19）.

nih.gov

ncbi.nlm.nih.gov

Gilmore, Gerry. The Short Spectacular Life of a Superstar. Science. 2004, 304 (5697): 1915–1916 [2007-05-01]. PMID 15218132. doi:10.1126/science.1100370. （原始内容存档于2009-02-01）.
Kroupa, Pavel. The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems. Science. 2002, 295 (5552): 82–91 [2007-12-03]. PMID 11778039. doi:10.1126/science.1067524. （原始内容存档于2009-11-25）.
Schilling, Govert. New Model Shows Sun Was a Hot Young Star. Science. 2001, 293 (5538): 2188–2189 [2007-02-04]. PMID 11567116. doi:10.1126/science.293.5538.2188. （原始内容存档于2009-01-31）.
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.
Krauss, Lawrence M.; Chaboyer, Brian. Age Estimates of Globular Clusters in the Milky Way: Constraints on Cosmology. Science. 2003, 299 (5603): 65–69. PMID 12511641. doi:10.1126/science.1075631.

rit.edu

spiff.rit.edu

Richmond, Michael W. Stellar evolution on the main sequence. Rochester Institute of Technology. 2004-11-10 [2007-12-03]. （原始内容存档于2020-05-12）.

sciencemag.org

Gilmore, Gerry. The Short Spectacular Life of a Superstar. Science. 2004, 304 (5697): 1915–1916 [2007-05-01]. PMID 15218132. doi:10.1126/science.1100370. （原始内容存档于2009-02-01）.
Kroupa, Pavel. The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems. Science. 2002, 295 (5552): 82–91 [2007-12-03]. PMID 11778039. doi:10.1126/science.1067524. （原始内容存档于2009-11-25）.
Schilling, Govert. New Model Shows Sun Was a Hot Young Star. Science. 2001, 293 (5538): 2188–2189 [2007-02-04]. PMID 11567116. doi:10.1126/science.293.5538.2188. （原始内容存档于2009-01-31）.

st-and.ac.uk

www-star.st-and.ac.uk

A course on stars' physical properties, formation and evolution (PDF). University of St. Andrews. [2010-05-18]. （原始内容存档 (PDF)于2020-12-02）.

swin.edu.au

astronomy.swin.edu.au

Zero Age Main Sequence. The SAO Encyclopedia of Astronomy. Swinburne University. [2007-12-09]. （原始内容存档于2018-10-19）.
White Dwarf. COSMOS—The SAO Encyclopedia of Astronomy. Swinburne University. [2007-12-04]. （原始内容存档于2017-09-26）.

u-strasbg.fr

simbad.u-strasbg.fr

SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. [2008-11-21]. （原始内容存档于2019-05-30）.
LTT 2151 -- High proper-motion Star. Centre de Données astronomiques de Strasbourg. [2008-08-12]. （原始内容存档于2019-05-12）.

uc.edu

physics.uc.edu

Sitko, Michael L. Stellar Structure and Evolution. University of Cincinnati. 2000-03-24 [2007-12-05]. （原始内容存档于2009-08-23）.

ucsd.edu

cass.ucsd.edu

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）.

ulb.ac.be

www-astro.ulb.ac.be

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.

unl.edu

astro.unl.edu

Origin of the Hertzsprung-Russell Diagram. University of Nebraska. [2007-12-06]. （原始内容存档于2011-07-16）.

uoregon.edu

zebu.uoregon.edu

Imamura, James N. Mass-Luminosity Relationship. University of Oregon. 1995-02-07 [2007-01-08]. （原始内容存档于2006-12-14）.

web.archive.org

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）.
Richard Powell. The Hertzsprung Russell Diagram. An Atlas of the Universe. 2006 [2009-10-29]. （原始内容存档于2010-12-31）.
Gilmore, Gerry. The Short Spectacular Life of a Superstar. Science. 2004, 304 (5697): 1915–1916 [2007-05-01]. PMID 15218132. doi:10.1126/science.1100370. （原始内容存档于2009-02-01）.
Morgan, W. W.; Keenan, P. C.; Kellman, E. An atlas of stellar spectra, with an outline of spectral classification. Chicago, Illinois: The University of Chicago press. 1943 [2008-08-12]. （原始内容存档于2011-05-14）.
Kroupa, Pavel. The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems. Science. 2002, 295 (5552): 82–91 [2007-12-03]. PMID 11778039. doi:10.1126/science.1067524. （原始内容存档于2009-11-25）.
Schilling, Govert. New Model Shows Sun Was a Hot Young Star. Science. 2001, 293 (5538): 2188–2189 [2007-02-04]. PMID 11567116. doi:10.1126/science.293.5538.2188. （原始内容存档于2009-01-31）.
Zero Age Main Sequence. The SAO Encyclopedia of Astronomy. Swinburne University. [2007-12-09]. （原始内容存档于2018-10-19）.
Main Sequence Stars. Australia Telescope Outreach and Education. [2007-12-04]. （原始内容存档于2013-12-29）.
White Dwarf. COSMOS—The SAO Encyclopedia of Astronomy. Swinburne University. [2007-12-04]. （原始内容存档于2017-09-26）.
Origin of the Hertzsprung-Russell Diagram. University of Nebraska. [2007-12-06]. （原始内容存档于2011-07-16）.
A course on stars' physical properties, formation and evolution (PDF). University of St. Andrews. [2010-05-18]. （原始内容存档 (PDF)于2020-12-02）.
Zombeck, Martin V. Handbook of Space Astronomy and Astrophysics 2nd. Cambridge University Press. 1990 [2007-12-06]. ISBN 0-521-34787-4. （原始内容存档于2010-12-29）.
SIMBAD Astronomical Database. Centre de Données astronomiques de Strasbourg. [2008-11-21]. （原始内容存档于2019-05-30）.
LTT 2151 -- High proper-motion Star. Centre de Données astronomiques de Strasbourg. [2008-08-12]. （原始内容存档于2019-05-12）.
Staff. List of the Nearest Hundred Nearest Star Systems. Research Consortium on Nearby Stars. 2008-01-01 [2008-08-12]. （原始内容存档于2012-05-13）.
Brainerd, Jerome James. Main-Sequence Stars. The Astrophysics Spectator. 2005-02-16 [2007-12-04]. （原始内容存档于2016-06-14）.
Lochner, Jim; Gibb, Meredith; Newman, Phil. Stars. NASA. 2006-09-06 [2007-12-05]. （原始内容存档于2014-11-19）.
Richmond, Michael W. Stellar evolution on the main sequence. Rochester Institute of Technology. 2004-11-10 [2007-12-03]. （原始内容存档于2020-05-12）.
For a detailed historical reconstruction of the theoretical derivation of this relationship by Eddington in 1924, see: Lecchini, Stefano. How Dwarfs Became Giants. The Discovery of the Mass-Luminosity Relation. Bern Studies in the History and Philosophy of Science. 2007 [2011-04-15]. ISBN 3-9522882-6-8. （原始内容存档于2022-11-09）.
Imamura, James N. Mass-Luminosity Relationship. University of Oregon. 1995-02-07 [2007-01-08]. （原始内容存档于2006-12-14）.
Sitko, Michael L. Stellar Structure and Evolution. University of Cincinnati. 2000-03-24 [2007-12-05]. （原始内容存档于2009-08-23）.
Staff. Post-Main Sequence Stars. Australia Telescope Outreach and Education. 2006-10-12 [2008-01-08]. （原始内容存档于2013-01-20）.

worldcat.org

Brown, Laurie M.; Pais, Abraham; Pippard, A. B. (编). Twentieth Century Physics. Bristol; New York: Institute of Physics, American Institute of Physics. 1995: 1696. ISBN 0-7503-0310-7. OCLC 33102501.