白色矮星 - 暇つぶしWikipedia

白色矮星

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2011年10月17日閲覧。
^ a b c d White Dwarfs, E. Schatzman, Amsterdam: North-Holland, 1958.
^ “The One Hundred Nearest Star Systems”. Research Consortium on Nearby Stars (2009年1月1日). 12 November 2007-11-12時点の ⇒オリジナルよりアーカイブ。2020年11月24日閲覧。
^ Ledrew, Glenn (2001). “The Real Starry Sky”. Journal of the Royal Astronomical Society of Canada 95: 32. https://ui.adsabs.harvard.edu/abs/2001JRASC..95...32L/abstract.
^ a b c d Fontaine, G.; Brassard, P.; Bergeron, P. (2001). “The Potential of White Dwarf Cosmochronology”. Publications of the Astronomical Society of the Pacific 113 (782): 409?435. Bibcode: 2001PASP..113..409F. doi:10.1086/319535.
^ a b c d e “Late stages of evolution for low-mass stars”. Lecture notes, Physics 230. Rochester Institute of Technology. 2017年9月4日時点の ⇒オリジナルよりアーカイブ。2007年3月3日閲覧。
^ a b Werner, K.; Hammer, N. J.; Nagel, T.; Rauch, T.; Dreizler, S. (2005). “On Possible Oxygen/Neon White Dwarfs: H1504+65 and the White Dwarf Donors in Ultracompact X-ray Binaries”. 14th European Workshop on White Dwarfs 334: 165. arXiv:astro-ph/0410690. Bibcode: 2005ASPC..334..165W.
^ a b Liebert, J.; Bergeron, P.; Eisenstein, D.; Harris, H. C.; Kleinman, S. J.; Nitta, A.; Krzesinski, J. (2004). “A Helium White Dwarf of Extremely Low Mass”. The Astrophysical Journal 606 (2): L147. arXiv:astro-ph/0404291. Bibcode: 2004ApJ...606L.147L. doi:10.1086/421462.
^ a b ⇒"Cosmic weight loss: The lowest mass white dwarf" (Press release). Harvard-Smithsonian Center for Astrophysics. 17 April 2007. 2007年4月22日時点のオリジナルよりアーカイブ。2007年4月20日閲覧。
^ a b Spergel, D. N.; Bean, R.; Dore, O.; Nolta, M. R.; Bennett, C. L.; Dunkley, J.; Hinshaw, G.; Jarosik, N. et al. (2007). “Three‐Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology”. The Astrophysical Journal Supplement Series 170 (2): 377?408. arXiv:astro-ph/0603449. Bibcode: 2007ApJS..170..377S. doi:10.1086/513700. ISSN 0067-0049.
^ Herschel, W. (1785). “Catalogue of Double Stars. By William Herschel, Esq. F. R. S”. Philosophical Transactions of the Royal Society of London 75: 40?126. Bibcode: 1785RSPT...75...40H. doi:10.1098/rstl.1785.0006. JSTOR 106749. https://www.semanticscholar.org/paper/760153d9a065023aa20cdea65e4734533c953e62.
^ a b c Holberg, J. B. (2005). How Degenerate Stars Came to be Known as White Dwarfs. 207. p. 1503. Bibcode: 2005AAS...20720501H.
^ Adams, W. S. (1914). “An A-Type Star of Very Low Luminosity”. Publications of the Astronomical Society of the Pacific 26: 198. Bibcode: 1914PASP...26..198A. doi:10.1086/122337. ISSN 0004-6280.
^ a b Bessel, F. W. (1844). “On the variations of the proper motions of Procyon and Sirius”. Monthly Notices of the Royal Astronomical Society 6 (11): 136?141. Bibcode: 1844MNRAS...6R.136B. doi:10.1093/mnras/6.11.136a.
^ a b Flammarion, Camille (1877). “The Companion of Sirius”. Astronomical Register 15: 186. Bibcode: 1877AReg...15..186F.
^ Adams, W. S. (1915). “The Spectrum of the Companion of Sirius”. Publications of the Astronomical Society of the Pacific 27: 236. Bibcode: 1915PASP...27..236A. doi:10.1086/122440. ISSN 0004-6280.
^ van Maanen, A. (1917). “Two Faint Stars with Large Proper Motion”. Publications of the Astronomical Society of the Pacific 29: 258. Bibcode: 1917PASP...29..258V. doi:10.1086/122654. ISSN 0004-6280.
^ Luyten, W. J. (1922). “The Mean Parallax of Early-Type Stars of Determined Proper Motion and Apparent Magnitude”. Publications of the Astronomical Society of the Pacific 34: 156. Bibcode: 1922PASP...34..156L. doi:10.1086/123176. ISSN 0004-6280.

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