飛馬座IK (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "飛馬座IK" in Chinese language version.

refsWebsite

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29harvard.edu

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15doi.org

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7arxiv.org

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2livingreviews.org

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2nasa.gov

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1iop.org

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1utk.edu

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1csiro.au

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1gsu.edu

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1cseligman.com

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1rit.edu

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1daviddarling.info

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1hubblesite.org

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1nih.gov

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1uoregon.edu

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aavso.org

Templeton, Matthew, Variable Star of the Season: Delta Scuti and the Delta Scuti variables, AAVSO, 2004 [2007-01-23], （原始内容存档于2006-10-26）（页面存档备份，存于互联网档案馆）
Malatesta, K.; Davis, K., Variable Star Of The Month: A Historical Look at Novae, AAVSO, May 2001 [2007-05-20], （原始内容存档于2007-05-19）（页面存档备份，存于互联网档案馆）
Malatesta, Kerri, Variable Star Of The Month—May, 2000: RS Ophiuchi, AAVSO, May 2000 [2007-05-15], （原始内容存档于2007-04-05）（页面存档备份，存于互联网档案馆）

archive.org

絕對星等M_v的表達式為：
M_v = V + 5(log₁₀ π + 1) = 2.762
其中V為視星等，π為視差。見：
Tayler, Roger John. The Stars: Their Structure and Evolution. Cambridge University Press. 1994: 16. ISBN 0-521-45885-4.

archive.today

淨自行量的表達式為：
${\begin{smallmatrix}\mu ={\sqrt {{\mu _{\delta }}^{2}+{\mu _{\alpha }}^{2}\cdot \cos ^{2}\delta }}=77.63\,\end{smallmatrix}}$ mas/y.
其中 $\mu _{\alpha }$ 和 $\mu _{\delta }$ 分別為自行的RA和Dec.部分。最終橫向速度為：
V_t = μ·4.74 d (pc) = 16.9 km.
其中d(pc)為距離，單位為秒差距。見：
Majewski, Steven R. Stellar Motions. University of Virginia. 2006 [2007-05-14]. （原始内容存档于2012-01-25）. Archive.today的存檔，存档日期2012-01-25

arxiv.org

Burleigh, M. R.; et al, Resolving Sirius-like Binaries with the Hubble Space Telescope, Provencal, J. L.; Shipman, H. L.; MacDonald, J.; Goodchild, S. (编), Proceedings 12th European Workshop on White Dwarfs, San Francisco: Astronomy Society of the Pacific: 222, July 28–August 1, 1975, Bibcode:2001ASPC..226..222B, ISBN 1-58381-058-7, arXiv:astro-ph/0010181  请检查|date=中的日期值 (帮助)
Heger, A.; et al, §3, How Massive Single Stars End Their Life, Astrophysical Journal, 2003, 591 (1): 288–300, Bibcode:2003ApJ...591..288H, arXiv:astro-ph/0212469 , doi:10.1086/375341
Oberhummer, H.; Csótó, A.; Schlattl, H., Stellar Production Rates of Carbon and Its Abundance in the Universe, Science, 2000, 289 (5476): 88–90, Bibcode:2000Sci...289...88O, PMID 10884230, arXiv:astro-ph/0007178 , doi:10.1126/science.289.5476.88
Gil-Pons, P.; García-Berro, E., On the formation of oxygen-neon white dwarfs in close binary systems, Astronomy and Astrophysics, 2001, 375 (1): 87–99, Bibcode:2001astro.ph..6224G, arXiv:astro-ph/0106224 , doi:10.1051/0004-6361:20010828
Langer, N.; Deutschmann, A.; Wellstein, S.; Höflich, P., The evolution of main sequence star + white dwarf binary systems towards Type Ia supernovae, Astronomy and Astrophysics, 2000, 362: 1046–1064, Bibcode:2000astro.ph..8444L, arXiv:astro-ph/0008444 
Hansen, Brad M. S., Type Ia Supernovae and High-Velocity White Dwarfs, The Astrophysical Journal, 2003, 582 (2): 915–918, Bibcode:2002astro.ph..6152H, arXiv:astro-ph/0206152 , doi:10.1086/344782
Marietta, E.; Burrows, A.; Fryxell, B., Type Ia Supernova Explosions in Binary Systems: The Impact on the Secondary Star and Its Consequences, The Astrophysical Journal Supplement Series, 2000, 128 (2): 615–650, Bibcode:2000ApJS..128..615M, arXiv:astro-ph/9908116 , doi:10.1086/313392

books.google.com

Rabinowitz, Harold; Vogel, Suzanne, The manual of scientific style: a guide for authors, editors, and researchers, Academic Press: 364, 2009, ISBN 0-12-373980-2
Saha, Swapan K., Diffraction-limited imaging with large and moderate telescopes, World Scientific: 440, 2007, ISBN 981-270-777-8

citebase.org

Di Stefano, Rosanne, Luminous Supersoft X-Ray Sources as Progenitors of Type Ia Supernovae, J. Greiner (编), Proceedings of the International Workshop on Supersoft X-Ray Sources, Garching, Germany: Springer-Verlag, February 28–March 1, 1996 [2007-05-19], ISBN 3-540-61390-0, （原始内容 (PDF)存档于2007-10-23）请检查|date=中的日期值 (帮助) （页面存档备份，存于互联网档案馆）

cseligman.com

Seligman, Courtney, The Mass-Luminosity Diagram and the Lifetime of Main-Sequence Stars, 2007 [2007-05-14], （原始内容存档于2012-06-29）（页面存档备份，存于互联网档案馆）

csiro.au

outreach.atnf.csiro.au

有關恆星的顏色，請參見：The Colour of Stars. Australia Telescope Outreach and Education. 2004-12-21 [2007-09-26]. （原始内容存档于2012-03-10）.

daviddarling.info

Darling, David, Carbon burning, The Internet Encyclopedia of Science, [2007-08-15], （原始内容存档于2012-05-11）（页面存档备份，存于互联网档案馆）

doi.org

白矮星的質量集中分佈在0.58個太陽質量左右，而且只有2%（見：
Holberg, J. B.; Barstow, M. A.; Bruhweiler, F. C.; Cruise, A. M.; Penny, A. J. Sirius B: A New, More Accurate View. The Astrophysical Journal. 1998, 497 (2): 935–942. Bibcode:1998ApJ...497..935H. doi:10.1086/305489. ）的白矮星質量超過1個太陽質量。
Kurtz, D. W., Metallicism and pulsation - The marginal metallic line stars, Astrophysical Journal, 1978, 221: 869–880, Bibcode:1978ApJ...221..869K, doi:10.1086/156090
Landsman, W.; Simon, T.; Bergeron, P., The hot white-dwarf companions of HR 1608, HR 8210, and HD 15638, Publications of the Astronomical Society of the Pacific, 1999, 105 (690): 841–847, Bibcode:1993PASP..105..841L, doi:10.1086/133242
Vennes, S.; Christian, D. J.; Thorstensen, J. R., Hot White Dwarfs in the Extreme-Ultraviolet Explorer Survey. IV. DA White Dwarfs with Bright Companions, The Astrophysical Journal, 1998, 502 (2): 763–787 [2010-01-05], Bibcode:1998ApJ...502..763V, doi:10.1086/305926, （原始内容存档于2020-06-14）（页面存档备份，存于互联网档案馆）
Vallerga, John, The Stellar Extreme-Ultraviolet Radiation Field, Astrophysical Journal, 1998, 497 (2): 77–115, Bibcode:1998ApJ...497..921V, doi:10.1086/305496
Paolo A. Mazzali, Friedrich K. Röpke, Stefano Benetti, Wolfgang Hillebrandt. A Common Explosion Mechanism for Type Ia Supernovae. Science. 2007-02-09, 315 (5813): 825–828 [2018-04-02]. ISSN 0036-8075. doi:10.1126/science.1136259. （原始内容存档于2021-05-23）（英语）. （页面存档备份，存于互联网档案馆）
Gautschy, A.; Saio, H., Stellar Pulsations Across The HR Diagram: Part 1, Annual Review of Astronomy and Astrophysics, 1995, 33 (1): 75–114, Bibcode:1995ARA&A..33...75G, doi:10.1146/annurev.aa.33.090195.000451
Heger, A.; et al, §3, How Massive Single Stars End Their Life, Astrophysical Journal, 2003, 591 (1): 288–300, Bibcode:2003ApJ...591..288H, arXiv:astro-ph/0212469 , doi:10.1086/375341
Oberhummer, H.; Csótó, A.; Schlattl, H., Stellar Production Rates of Carbon and Its Abundance in the Universe, Science, 2000, 289 (5476): 88–90, Bibcode:2000Sci...289...88O, PMID 10884230, arXiv:astro-ph/0007178 , doi:10.1126/science.289.5476.88
Iben, Icko, Jr., Single and binary star evolution, Astrophysical Journal Supplement Series, 1991, 76: 55–114, Bibcode:1991ApJS...76...55I, doi:10.1086/191565
Gil-Pons, P.; García-Berro, E., On the formation of oxygen-neon white dwarfs in close binary systems, Astronomy and Astrophysics, 2001, 375 (1): 87–99, Bibcode:2001astro.ph..6224G, arXiv:astro-ph/0106224 , doi:10.1051/0004-6361:20010828
Woosley, S. E.; Heger, A., The Evolution and Explosion of Massive Stars (PDF), Reviews of Modern Physics, 2002, 74 (4): 1015–1071 [2007-05-30], Bibcode:2002RvMP...74.1015W, doi:10.1103/RevModPhys.74.1015, （原始内容 (PDF)存档于2012-03-18）（页面存档备份，存于互联网档案馆）
Beech, Martin, The past, present and future supernova threat to Earth's biosphere, Astrophysics and Space Science (Springer), 2011 [2011-11-15], Bibcode:2011Ap&SS.336..287B, doi:10.1007/s10509-011-0873-9 ^{[永久失效連結]}
Hansen, Brad M. S., Type Ia Supernovae and High-Velocity White Dwarfs, The Astrophysical Journal, 2003, 582 (2): 915–918, Bibcode:2002astro.ph..6152H, arXiv:astro-ph/0206152 , doi:10.1086/344782
Marietta, E.; Burrows, A.; Fryxell, B., Type Ia Supernova Explosions in Binary Systems: The Impact on the Secondary Star and Its Consequences, The Astrophysical Journal Supplement Series, 2000, 128 (2): 615–650, Bibcode:2000ApJS..128..615M, arXiv:astro-ph/9908116 , doi:10.1086/313392

gsu.edu

hyperphysics.phy-astr.gsu.edu

Anonymous, Stellar Lifetimes, Georgia State University, 2005 [2007-02-26], （原始内容存档于2012-06-15）（页面存档备份，存于互联网档案馆）

harvard.edu

ui.adsabs.harvard.edu

白矮星的質量集中分佈在0.58個太陽質量左右，而且只有2%（見：
Holberg, J. B.; Barstow, M. A.; Bruhweiler, F. C.; Cruise, A. M.; Penny, A. J. Sirius B: A New, More Accurate View. The Astrophysical Journal. 1998, 497 (2): 935–942. Bibcode:1998ApJ...497..935H. doi:10.1086/305489. ）的白矮星質量超過1個太陽質量。
Kurtz, D. W., Metallicism and pulsation - The marginal metallic line stars, Astrophysical Journal, 1978, 221: 869–880, Bibcode:1978ApJ...221..869K, doi:10.1086/156090
Barstow, M. A.; Holberg, J. B.; Koester, D., Extreme Ultraviolet Spectrophotometry of HD16538 and HR:8210 Ik-Pegasi, Monthly Notices of the Royal Astronomical Society, 1994, 270 (3): 516, Bibcode:1994MNRAS.270..516B
Wonnacott, D.; Kellett, B. J.; Smalley, B.; Lloyd, C., Pulsational Activity on Ik-Pegasi, Monthly Notices of the Royal Astronomical Society, 1994, 267 (4): 1045–1052, Bibcode:1994MNRAS.267.1045W
Landsman, W.; Simon, T.; Bergeron, P., The hot white-dwarf companions of HR 1608, HR 8210, and HD 15638, Publications of the Astronomical Society of the Pacific, 1999, 105 (690): 841–847, Bibcode:1993PASP..105..841L, doi:10.1086/133242
Smalley, B.; et al, The chemical composition of IK Pegasi, Monthly Notices of the Royal Astronomical Society, 1996, 278 (3): 688–696, Bibcode:1996MNRAS.278..688S
Vennes, S.; Christian, D. J.; Thorstensen, J. R., Hot White Dwarfs in the Extreme-Ultraviolet Explorer Survey. IV. DA White Dwarfs with Bright Companions, The Astrophysical Journal, 1998, 502 (2): 763–787 [2010-01-05], Bibcode:1998ApJ...502..763V, doi:10.1086/305926, （原始内容存档于2020-06-14）（页面存档备份，存于互联网档案馆）
Vallerga, John, The Stellar Extreme-Ultraviolet Radiation Field, Astrophysical Journal, 1998, 497 (2): 77–115, Bibcode:1998ApJ...497..921V, doi:10.1086/305496
Wonnacott, D.; Kellett, B. J.; Stickland, D. J., IK Peg - A nearby, short-period, Sirius-like system, Monthly Notices of the Royal Astronomical Society, 1993, 262 (2): 277–284, Bibcode:1993MNRAS.262..277W
Pickering, Edward Charles, Revised Harvard photometry: a catalogue of the positions, photometric magnitudes and spectra of 9110 stars, mainly of the magnitude 6.50, and brighter observed with the 2 and 4-英寸（100-毫米） meridian photometers, Annals of the Astronomical Observatory of Harvard College, 1908, 50: 182, Bibcode:1908AnHar..50....1P
Harper, W. E., The orbits of A Persei and HR 8210, Publications of the Dominion Astrophysical Observatory, 1927, 4: 161–169, Bibcode:1927PDAO....4..161H
Perryman, M. A. C.; et al, The Hipparcos Catalogue, Astronomy & Astrophysics, 1997, 323: L49–L52, Bibcode:1997A&A...323L..49P
Wilson, Ralph Elmer, General catalogue of stellar radial velocities, Carnegie Institution of Washington, 1953, Bibcode:1953QB901.W495.....
Burleigh, M. R.; et al, Resolving Sirius-like Binaries with the Hubble Space Telescope, Provencal, J. L.; Shipman, H. L.; MacDonald, J.; Goodchild, S. (编), Proceedings 12th European Workshop on White Dwarfs, San Francisco: Astronomy Society of the Pacific: 222, July 28–August 1, 1975, Bibcode:2001ASPC..226..222B, ISBN 1-58381-058-7, arXiv:astro-ph/0010181  请检查|date=中的日期值 (帮助)
Gautschy, A.; Saio, H., Stellar Pulsations Across The HR Diagram: Part 1, Annual Review of Astronomy and Astrophysics, 1995, 33 (1): 75–114, Bibcode:1995ARA&A..33...75G, doi:10.1146/annurev.aa.33.090195.000451
Mayer, J. G.; Hakkila, J., Photometric Effects of Binarity on AM Star Broadband Colors, Bulletin of the American Astronomical Society, 1994, 26: 868, Bibcode:1994AAS...184.0607M
Heger, A.; et al, §3, How Massive Single Stars End Their Life, Astrophysical Journal, 2003, 591 (1): 288–300, Bibcode:2003ApJ...591..288H, arXiv:astro-ph/0212469 , doi:10.1086/375341
Oberhummer, H.; Csótó, A.; Schlattl, H., Stellar Production Rates of Carbon and Its Abundance in the Universe, Science, 2000, 289 (5476): 88–90, Bibcode:2000Sci...289...88O, PMID 10884230, arXiv:astro-ph/0007178 , doi:10.1126/science.289.5476.88
Iben, Icko, Jr., Single and binary star evolution, Astrophysical Journal Supplement Series, 1991, 76: 55–114, Bibcode:1991ApJS...76...55I, doi:10.1086/191565
Gil-Pons, P.; García-Berro, E., On the formation of oxygen-neon white dwarfs in close binary systems, Astronomy and Astrophysics, 2001, 375 (1): 87–99, Bibcode:2001astro.ph..6224G, arXiv:astro-ph/0106224 , doi:10.1051/0004-6361:20010828
Woosley, S. E.; Heger, A., The Evolution and Explosion of Massive Stars (PDF), Reviews of Modern Physics, 2002, 74 (4): 1015–1071 [2007-05-30], Bibcode:2002RvMP...74.1015W, doi:10.1103/RevModPhys.74.1015, （原始内容 (PDF)存档于2012-03-18）（页面存档备份，存于互联网档案馆）
Langer, N.; Deutschmann, A.; Wellstein, S.; Höflich, P., The evolution of main sequence star + white dwarf binary systems towards Type Ia supernovae, Astronomy and Astrophysics, 2000, 362: 1046–1064, Bibcode:2000astro.ph..8444L, arXiv:astro-ph/0008444 
Langer, N.; Yoon, S.-C.; Wellstein, S.; Scheithauer, S., On the evolution of interacting binaries which contain a white dwarf, Gänsicke, B. T.; Beuermann, K.; Rein, K. (编), The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, San Francisco, California: Astronomical Society of the Pacific: 252, 2002, Bibcode:2002ASPC..261..252L
Beech, Martin, The past, present and future supernova threat to Earth's biosphere, Astrophysics and Space Science (Springer), 2011 [2011-11-15], Bibcode:2011Ap&SS.336..287B, doi:10.1007/s10509-011-0873-9 ^{[永久失效連結]}
Hansen, Brad M. S., Type Ia Supernovae and High-Velocity White Dwarfs, The Astrophysical Journal, 2003, 582 (2): 915–918, Bibcode:2002astro.ph..6152H, arXiv:astro-ph/0206152 , doi:10.1086/344782
Marietta, E.; Burrows, A.; Fryxell, B., Type Ia Supernova Explosions in Binary Systems: The Impact on the Secondary Star and Its Consequences, The Astrophysical Journal Supplement Series, 2000, 128 (2): 615–650, Bibcode:2000ApJS..128..615M, arXiv:astro-ph/9908116 , doi:10.1086/313392

chandra.harvard.edu

Staff, White Dwarfs & Planetary Nebulas, Harvard-Smithsonian Center for Astrophysics, 2006-08-29 [2007-06-09], （原始内容存档于2012-06-23）（页面存档备份，存于互联网档案馆）
Staff, Stellar Evolution - Cycles of Formation and Destruction, Harvard-Smithsonian Center for Astrophysics, 2006-08-29 [2006-08-10], （原始内容存档于2012-05-05）（页面存档备份，存于互联网档案馆）
Staff, Stellar Evolution - Cycles of Formation and Destruction, Harvard-Smithsonian Center for Astrophysics, 2006-08-29 [2006-08-10], （原始内容存档于2012-05-05）（页面存档备份，存于互联网档案馆）

hsc.edu

ceres.hsc.edu

根據：
${\begin{smallmatrix}{\frac {L}{L_{sun}}}=\left({\frac {R}{R_{sun}}}\right)^{2}\left({\frac {T_{eff}}{T_{sun}}}\right)^{4}\end{smallmatrix}}$
其中L為光度，R為半徑，T_eff為溫度。見：
Krimm, Hans. Luminosity, Radius and Temperature. Hampden-Sydney College. 1997-08-19 [2007-05-16]. （原始内容存档于2003-05-08）. （页面存档备份，存于互联网档案馆）

hubblesite.org

Savage, D.; Jones, T.; Villard, Ray; Watzke, M., Hubble Separates Stars in the Mira Binary System, HubbleSite News Center, 1997-08-06 [2007-03-01], （原始内容存档于2012-04-02）（页面存档备份，存于互联网档案馆）

iop.org

Vennes, S.; Christian, D. J.; Thorstensen, J. R., Hot White Dwarfs in the Extreme-Ultraviolet Explorer Survey. IV. DA White Dwarfs with Bright Companions, The Astrophysical Journal, 1998, 502 (2): 763–787 [2010-01-05], Bibcode:1998ApJ...502..763V, doi:10.1086/305926, （原始内容存档于2020-06-14）（页面存档备份，存于互联网档案馆）

livingreviews.org

relativity.livingreviews.org

Postnov, K. A.; Yungelson, L. R., The Evolution of Compact Binary Star Systems, Living Reviews in Relativity, 2006 [2007-05-16], （原始内容存档于2007-09-26）（页面存档备份，存于互联网档案馆）
Fryer, C. L.; New, K. C. B., 2.1 Collapse scenario, Gravitational Waves from Gravitational Collapse (Max-Planck-Gesellschaft), 2006-01-24 [2007-06-07], （原始内容存档于2011-03-27）（页面存档备份，存于互联网档案馆）

nasa.gov

Hendrix, Susan, Scientists see Storm Before the Storm in Future Supernova, NASA, 2007-07-20 [2007-05-25], （原始内容存档于2021-05-19）（页面存档备份，存于互联网档案馆）

heasarc.gsfc.nasa.gov

Staff, Introduction to Supernova Remnants, NASA/Goddard, 2006-09-07 [2007-05-20], （原始内容存档于2020-05-28）（页面存档备份，存于互联网档案馆）

nih.gov

ncbi.nlm.nih.gov

Oberhummer, H.; Csótó, A.; Schlattl, H., Stellar Production Rates of Carbon and Its Abundance in the Universe, Science, 2000, 289 (5476): 88–90, Bibcode:2000Sci...289...88O, PMID 10884230, arXiv:astro-ph/0007178 , doi:10.1126/science.289.5476.88

rit.edu

spiff.rit.edu

Richmond, Michael, Late stages of evolution for low-mass stars, Rochester Institute of Technology, 2006-10-05 [2007-06-07], （原始内容存档于2020-06-11）（页面存档备份，存于互联网档案馆）

sciencebits.com

Estimating Stellar Parameters from Energy Equipartition, ScienceBits, [2007-05-15], （原始内容存档于2012-05-22）（页面存档备份，存于互联网档案馆）

sciencemag.org

science.sciencemag.org

Paolo A. Mazzali, Friedrich K. Röpke, Stefano Benetti, Wolfgang Hillebrandt. A Common Explosion Mechanism for Type Ia Supernovae. Science. 2007-02-09, 315 (5813): 825–828 [2018-04-02]. ISSN 0036-8075. doi:10.1126/science.1136259. （原始内容存档于2021-05-23）（英语）. （页面存档备份，存于互联网档案馆）

springerlink.com

Beech, Martin, The past, present and future supernova threat to Earth's biosphere, Astrophysics and Space Science (Springer), 2011 [2011-11-15], Bibcode:2011Ap&SS.336..287B, doi:10.1007/s10509-011-0873-9 ^{[永久失效連結]}

tass-survey.org

Richmond, Michael, Will a Nearby Supernova Endanger Life on Earth?, 2005-04-08 [2006-03-30], （原始内容 (TXT)存档于2007-03-06）（页面存档备份，存于互联网档案馆）—see section 4.

u-strasbg.fr

simbad.u-strasbg.fr

SIMBAD Query Result: HD 204188 -- Spectroscopic binary, SIMBAD (Centre de Données astronomiques de Strasbourg), [2009-01-02], （原始内容存档于2013-11-03）（页面存档备份，存于互联网档案馆） — 註：某些結果需通過網頁中的「Display all measurements」功能取得。

ucolick.org

Woosley, S. E.; Heger, A., The Evolution and Explosion of Massive Stars (PDF), Reviews of Modern Physics, 2002, 74 (4): 1015–1071 [2007-05-30], Bibcode:2002RvMP...74.1015W, doi:10.1103/RevModPhys.74.1015, （原始内容 (PDF)存档于2012-03-18）（页面存档备份，存于互联网档案馆）

uoregon.edu

zebu.uoregon.edu

Imamura, James N., Cooling of White Dwarfs, University of Oregon, 1995-02-24 [2007-05-19], （原始内容存档于2007-05-02）（页面存档备份，存于互联网档案馆）

utk.edu

csep10.phys.utk.edu

Staff, Spectroscopic Binaries, University of Tennessee, [2007-06-09], （原始内容存档于2012-07-05）（页面存档备份，存于互联网档案馆）

virginia.edu

astro.virginia.edu

淨自行量的表達式為：
${\begin{smallmatrix}\mu ={\sqrt {{\mu _{\delta }}^{2}+{\mu _{\alpha }}^{2}\cdot \cos ^{2}\delta }}=77.63\,\end{smallmatrix}}$ mas/y.
其中 $\mu _{\alpha }$ 和 $\mu _{\delta }$ 分別為自行的RA和Dec.部分。最終橫向速度為：
V_t = μ·4.74 d (pc) = 16.9 km.
其中d(pc)為距離，單位為秒差距。見：
Majewski, Steven R. Stellar Motions. University of Virginia. 2006 [2007-05-14]. （原始内容存档于2012-01-25）. Archive.today的存檔，存档日期2012-01-25

web.archive.org

根據：
${\begin{smallmatrix}{\frac {L}{L_{sun}}}=\left({\frac {R}{R_{sun}}}\right)^{2}\left({\frac {T_{eff}}{T_{sun}}}\right)^{4}\end{smallmatrix}}$
其中L為光度，R為半徑，T_eff為溫度。見：
Krimm, Hans. Luminosity, Radius and Temperature. Hampden-Sydney College. 1997-08-19 [2007-05-16]. （原始内容存档于2003-05-08）. （页面存档备份，存于互联网档案馆）
SIMBAD Query Result: HD 204188 -- Spectroscopic binary, SIMBAD (Centre de Données astronomiques de Strasbourg), [2009-01-02], （原始内容存档于2013-11-03）（页面存档备份，存于互联网档案馆） — 註：某些結果需通過網頁中的「Display all measurements」功能取得。
Vennes, S.; Christian, D. J.; Thorstensen, J. R., Hot White Dwarfs in the Extreme-Ultraviolet Explorer Survey. IV. DA White Dwarfs with Bright Companions, The Astrophysical Journal, 1998, 502 (2): 763–787 [2010-01-05], Bibcode:1998ApJ...502..763V, doi:10.1086/305926, （原始内容存档于2020-06-14）（页面存档备份，存于互联网档案馆）
Paolo A. Mazzali, Friedrich K. Röpke, Stefano Benetti, Wolfgang Hillebrandt. A Common Explosion Mechanism for Type Ia Supernovae. Science. 2007-02-09, 315 (5813): 825–828 [2018-04-02]. ISSN 0036-8075. doi:10.1126/science.1136259. （原始内容存档于2021-05-23）（英语）. （页面存档备份，存于互联网档案馆）
Staff, Spectroscopic Binaries, University of Tennessee, [2007-06-09], （原始内容存档于2012-07-05）（页面存档备份，存于互联网档案馆）
Templeton, Matthew, Variable Star of the Season: Delta Scuti and the Delta Scuti variables, AAVSO, 2004 [2007-01-23], （原始内容存档于2006-10-26）（页面存档备份，存于互联网档案馆）
Anonymous, Stellar Lifetimes, Georgia State University, 2005 [2007-02-26], （原始内容存档于2012-06-15）（页面存档备份，存于互联网档案馆）
Staff, White Dwarfs & Planetary Nebulas, Harvard-Smithsonian Center for Astrophysics, 2006-08-29 [2007-06-09], （原始内容存档于2012-06-23）（页面存档备份，存于互联网档案馆）
Seligman, Courtney, The Mass-Luminosity Diagram and the Lifetime of Main-Sequence Stars, 2007 [2007-05-14], （原始内容存档于2012-06-29）（页面存档备份，存于互联网档案馆）
Staff, Stellar Evolution - Cycles of Formation and Destruction, Harvard-Smithsonian Center for Astrophysics, 2006-08-29 [2006-08-10], （原始内容存档于2012-05-05）（页面存档备份，存于互联网档案馆）
Richmond, Michael, Late stages of evolution for low-mass stars, Rochester Institute of Technology, 2006-10-05 [2007-06-07], （原始内容存档于2020-06-11）（页面存档备份，存于互联网档案馆）
Darling, David, Carbon burning, The Internet Encyclopedia of Science, [2007-08-15], （原始内容存档于2012-05-11）（页面存档备份，存于互联网档案馆）
Savage, D.; Jones, T.; Villard, Ray; Watzke, M., Hubble Separates Stars in the Mira Binary System, HubbleSite News Center, 1997-08-06 [2007-03-01], （原始内容存档于2012-04-02）（页面存档备份，存于互联网档案馆）
Woosley, S. E.; Heger, A., The Evolution and Explosion of Massive Stars (PDF), Reviews of Modern Physics, 2002, 74 (4): 1015–1071 [2007-05-30], Bibcode:2002RvMP...74.1015W, doi:10.1103/RevModPhys.74.1015, （原始内容 (PDF)存档于2012-03-18）（页面存档备份，存于互联网档案馆）
Estimating Stellar Parameters from Energy Equipartition, ScienceBits, [2007-05-15], （原始内容存档于2012-05-22）（页面存档备份，存于互联网档案馆）
Imamura, James N., Cooling of White Dwarfs, University of Oregon, 1995-02-24 [2007-05-19], （原始内容存档于2007-05-02）（页面存档备份，存于互联网档案馆）
Postnov, K. A.; Yungelson, L. R., The Evolution of Compact Binary Star Systems, Living Reviews in Relativity, 2006 [2007-05-16], （原始内容存档于2007-09-26）（页面存档备份，存于互联网档案馆）
Malatesta, K.; Davis, K., Variable Star Of The Month: A Historical Look at Novae, AAVSO, May 2001 [2007-05-20], （原始内容存档于2007-05-19）（页面存档备份，存于互联网档案馆）
Malatesta, Kerri, Variable Star Of The Month—May, 2000: RS Ophiuchi, AAVSO, May 2000 [2007-05-15], （原始内容存档于2007-04-05）（页面存档备份，存于互联网档案馆）
Hendrix, Susan, Scientists see Storm Before the Storm in Future Supernova, NASA, 2007-07-20 [2007-05-25], （原始内容存档于2021-05-19）（页面存档备份，存于互联网档案馆）
Di Stefano, Rosanne, Luminous Supersoft X-Ray Sources as Progenitors of Type Ia Supernovae, J. Greiner (编), Proceedings of the International Workshop on Supersoft X-Ray Sources, Garching, Germany: Springer-Verlag, February 28–March 1, 1996 [2007-05-19], ISBN 3-540-61390-0, （原始内容 (PDF)存档于2007-10-23）请检查|date=中的日期值 (帮助) （页面存档备份，存于互联网档案馆）
Fryer, C. L.; New, K. C. B., 2.1 Collapse scenario, Gravitational Waves from Gravitational Collapse (Max-Planck-Gesellschaft), 2006-01-24 [2007-06-07], （原始内容存档于2011-03-27）（页面存档备份，存于互联网档案馆）
Staff, Stellar Evolution - Cycles of Formation and Destruction, Harvard-Smithsonian Center for Astrophysics, 2006-08-29 [2006-08-10], （原始内容存档于2012-05-05）（页面存档备份，存于互联网档案馆）
Richmond, Michael, Will a Nearby Supernova Endanger Life on Earth?, 2005-04-08 [2006-03-30], （原始内容 (TXT)存档于2007-03-06）（页面存档备份，存于互联网档案馆）—see section 4.
Staff, Introduction to Supernova Remnants, NASA/Goddard, 2006-09-07 [2007-05-20], （原始内容存档于2020-05-28）（页面存档备份，存于互联网档案馆）

webcitation.org

淨自行量的表達式為：
${\begin{smallmatrix}\mu ={\sqrt {{\mu _{\delta }}^{2}+{\mu _{\alpha }}^{2}\cdot \cos ^{2}\delta }}=77.63\,\end{smallmatrix}}$ mas/y.
其中 $\mu _{\alpha }$ 和 $\mu _{\delta }$ 分別為自行的RA和Dec.部分。最終橫向速度為：
V_t = μ·4.74 d (pc) = 16.9 km.
其中d(pc)為距離，單位為秒差距。見：
Majewski, Steven R. Stellar Motions. University of Virginia. 2006 [2007-05-14]. （原始内容存档于2012-01-25）. Archive.today的存檔，存档日期2012-01-25
有關恆星的顏色，請參見：The Colour of Stars. Australia Telescope Outreach and Education. 2004-12-21 [2007-09-26]. （原始内容存档于2012-03-10）.

worldcat.org

Paolo A. Mazzali, Friedrich K. Röpke, Stefano Benetti, Wolfgang Hillebrandt. A Common Explosion Mechanism for Type Ia Supernovae. Science. 2007-02-09, 315 (5813): 825–828 [2018-04-02]. ISSN 0036-8075. doi:10.1126/science.1136259. （原始内容存档于2021-05-23）（英语）. （页面存档备份，存于互联网档案馆）