錢德拉塞卡極限 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "錢德拉塞卡極限" in Chinese language version.

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9web.archive.org

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7harvard.edu

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1doi.org

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1nobelprize.org

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1u-strasbg.fr

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arxiv.org

An Empirical Initial-Final Mass Relation from Hot, Massive White Dwarfs in NGC 2168 (M35) （页面存档备份，存于互联网档案馆）, Kurtis A. Williams, M. Bolte, and Detlev Koester, Astrophysical Journal 615, #1 (2004), pp. L49–L52; also arXiv astro-ph/0409447 （页面存档备份，存于互联网档案馆）.

doi.org

Mazzali, P. A.; K. Röpke, F. K.; Benetti, S.; Hillebrandt, W. A Common Explosion Mechanism for Type Ia Supernovae. Science. 2007, 315 (5813): 825–828. doi:10.1126/science.1136259.

harvard.edu

adsabs.harvard.edu

The Neutron Star and Black Hole Initial Mass Function （页面存档备份，存于互联网档案馆）, F. X. Timmes, S. E. Woosley, and Thomas A. Weaver, Astrophysical Journal 457 (February 1, 1996), pp. 834–843.
The Highly Collapsed Configurations of a Stellar Mass （页面存档备份，存于互联网档案馆）, S. Chandrasekhar, Monthly Notices of the Royal Astronomical Society 91 (1931), 456–466.
The Highly Collapsed Configurations of a Stellar Mass (second paper) （页面存档备份，存于互联网档案馆）, S. Chandrasekhar, Monthly Notices of the Royal Astronomical Society, 95 (1935), pp. 207--225.
White dwarfs in open clusters. VIII. NGC 2516: a test for the mass-radius and initial-final mass relations （页面存档备份，存于互联网档案馆）, D. Koester and D. Reimers, Astronomy and Astrophysics 313 (1996), pp. 810–814.
An Empirical Initial-Final Mass Relation from Hot, Massive White Dwarfs in NGC 2168 (M35) （页面存档备份，存于互联网档案馆）, Kurtis A. Williams, M. Bolte, and Detlev Koester, Astrophysical Journal 615, #1 (2004), pp. L49–L52; also arXiv astro-ph/0409447 （页面存档备份，存于互联网档案馆）.
How Massive Single Stars End Their Life （页面存档备份，存于互联网档案馆）, A. Heger, C. L. Fryer, S. E. Woosley, N. Langer, and D. H. Hartmann, Astrophysical Journal 591, #1 (2003), pp. 288–300.
The Maximum Mass of Ideal White Dwarfs （页面存档备份，存于互联网档案馆）, S. Chandrasekhar, Astrophysical Journal 74 (1931), pp. 81–82.

nobelprize.org

On Stars, Their Evolution and Their Stability （页面存档备份，存于互联网档案馆）, Nobel Prize lecture, Subrahmanyan Chandrasekhar, December 8, 1983.

u-strasbg.fr

vizier.u-strasbg.fr

Standards for Astronomical Catalogues, Version 2.0 （页面存档备份，存于互联网档案馆）, section 3.2.2, web page, accessed 12-I-2007.

web.archive.org

The Neutron Star and Black Hole Initial Mass Function （页面存档备份，存于互联网档案馆）, F. X. Timmes, S. E. Woosley, and Thomas A. Weaver, Astrophysical Journal 457 (February 1, 1996), pp. 834–843.
The Highly Collapsed Configurations of a Stellar Mass （页面存档备份，存于互联网档案馆）, S. Chandrasekhar, Monthly Notices of the Royal Astronomical Society 91 (1931), 456–466.
The Highly Collapsed Configurations of a Stellar Mass (second paper) （页面存档备份，存于互联网档案馆）, S. Chandrasekhar, Monthly Notices of the Royal Astronomical Society, 95 (1935), pp. 207--225.
On Stars, Their Evolution and Their Stability （页面存档备份，存于互联网档案馆）, Nobel Prize lecture, Subrahmanyan Chandrasekhar, December 8, 1983.
Standards for Astronomical Catalogues, Version 2.0 （页面存档备份，存于互联网档案馆）, section 3.2.2, web page, accessed 12-I-2007.
White dwarfs in open clusters. VIII. NGC 2516: a test for the mass-radius and initial-final mass relations （页面存档备份，存于互联网档案馆）, D. Koester and D. Reimers, Astronomy and Astrophysics 313 (1996), pp. 810–814.
An Empirical Initial-Final Mass Relation from Hot, Massive White Dwarfs in NGC 2168 (M35) （页面存档备份，存于互联网档案馆）, Kurtis A. Williams, M. Bolte, and Detlev Koester, Astrophysical Journal 615, #1 (2004), pp. L49–L52; also arXiv astro-ph/0409447 （页面存档备份，存于互联网档案馆）.
How Massive Single Stars End Their Life （页面存档备份，存于互联网档案馆）, A. Heger, C. L. Fryer, S. E. Woosley, N. Langer, and D. H. Hartmann, Astrophysical Journal 591, #1 (2003), pp. 288–300.
The Maximum Mass of Ideal White Dwarfs （页面存档备份，存于互联网档案馆）, S. Chandrasekhar, Astrophysical Journal 74 (1931), pp. 81–82.