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超新星候選列表

维基媒体列表条目

超新星候選列表是天文學家提出將成為超新星前身的恆星。II型超新星的前身包括演化至最後階段的質量仍然大於10倍太陽質量的恆星(在這個質量範圍內的恆星，著名的例子包括心宿二、角宿一[1]、天社一[2] 仙王座μ和五合星團中的一些成員[3]。)。Ia型超新星的前身是接近錢德拉塞卡極限，經由伴星吸積至大約是1.44太陽質量的白矮星。這張表也包括大質量的沃夫-瑞葉星，它們可能會成為Ia/Ib超新星。

本表是動態列表，或許永遠不會完結。歡迎您參考可靠來源來查漏補缺。
超新星前身候選者
名稱曆元 J2000星座距離
(光年)		光譜
分類		註解
R. A.Dec.
飛馬座IK21h 26m 26.7s+19° 22′ 32″飛馬座150A8m:/DA[4][5]
角宿一13h 25m 11.6s-11° 09′ 40.8″室女座250B1[6]
骑官十14h 41m 56s–47° 23′ 17″豺狼座550B1.5[7][6]
心宿二16h 29m 24s–26° 25′ 55″天蝎座600M1.5Iab-b[8][6]
参宿四05h 55m 10.3s+07° 24′ 25″獵戶座640M2Iab[1][9]
天社一08h 09m 32.0s−47° 20′ 12″船帆座800WC8[9]
参宿七05h 14m 32.3s–08° 12′ 06″猎户座860B8Ia[10][6]
弧矢九7h 17m 08s–37° 05′ 51″船尾座1,100K3 Ib
金牛座11905h 32m 12.8s+18° 35′ 40″金牛座1,700M2Iab-Ib
蛇夫座RS17h 50m 13.2s–06° 42′ 28″蛇夫座1,950–5,200M2III/D[11][12]
HD 16862518h 21m 19.5s−16° 22′ 26″人馬座7,200B6Ia[13]
羅盤座T09h 04m 41.5s−32° 22′ 48″羅盤座3,260[14][15]
HD 17982119h 13m 58.6s+00° 07′ 32″天鷹座3,300G5Ia[16][17]
大犬座VY07h 22m 58.3s−25° 46′ 03″大犬座4,900M5eIa[18][19]
Sher 2511h 15m 07.8s−61° 15′ 17″船底座~20,000B1.5Iab[20]
海山二10h 45m 03.6s−59° 41′ 04″船底座7,000–8,000B3-5Ia0/O7I(WC8)[21][22]
WR 10418h 02m 04.1s–23° 37′ 41″人馬座8,000WC9d/OB[23][24]
IRC+1042019h 26m 48.1s+11° 21′ 17″天鷹座10,000-23,000F8Ia+[25][26]
仙后座ρ23h 54m 23.0s+57° 29′ 58″仙后座12,000G2Ia0e[27]
HD 17982119h 13m 58.6s+00° 07′ 32″天鷹座20,000G5Ia[17][28]
船尾座V44507h 37m 56.9s–25° 56′ 59″船尾座27,000[29]
天蝎座U16h 22m 30.7s–17° 52′ 42″天蝎座39,000[30]
KPD1930+275219h 32m 14.9s+27° 58′ 35″天鵝座sdB/D[nb 1][31][32]

註解编辑

  1. ^ The Kitt Peak Downes star.

參考資料编辑

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  10. ^ Moravveji, Ehsan; Guinan, Edward F.; Shultz, Matt; Williamson, Michael H.; Moya, Andres, Asteroseismology of the nearby SN-II Progenitor: Rigel. Part I. The MOST High-precision Photometry and Radial Velocity Monitoring, The Astrophysical Journal, March 2012, 747 (1): 108–115, Bibcode:2012ApJ...747..108M, arXiv:1201.0843  , doi:10.1088/0004-637X/747/2/108 
  11. ^ Than, Ker. Mystery of Explosive Star Solved. space.com. 2006-07-19 [2007-01-08]. （原始内容存档于2010-05-28）. 
  12. ^ Staff. Astronomers See Future Supernova Developing. SpaceDaily. 2006-07-25 [2006-12-01]. （原始内容存档于2021-02-13）. 
  13. ^ Smith, Nathan. Discovery of a Nearby Twin of SN 1987A's Nebula around the Luminous Blue Variable HD 168625: Was Sk -69 202 an LBV?. The Astronomical Journal. March 2007, 133 (3): 1034–1040. Bibcode:2007AJ....133.1034S. doi:10.1086/510838. 
  14. ^ Schaefer, Bradley E.; Pagnotta, Ashley; Shara, Michael M. The Nova Shell and Evolution of the Recurrent Nova T Pyxidis. January 2010. Bibcode:2010ApJ...708..381S. doi:10.1088/0004-637X/708/1/381. 
  15. ^ Edwards, Lin. Massive white dwarf in our galaxy may go supernova. PhysOrg. 2010 [2010-02-26]. （原始内容存档于2012-01-27）. 
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  17. ^ 17.0 17.1 Josselin, E.; Lèbre, A. Probing the post-AGB nature of HD 179821. Astronomy and Astrophysics. 2001, 367: 826–830. doi:10.1051/0004-6361:20000496. 
  18. ^ Smith, Nathan; Hinkle, Kenneth H.; Ryde, Nils. Red Supergiants as Potential Type IIn Supernova Progenitors: Spatially Resolved 4.6 μm CO Emission Around VY CMa and Betelgeuse. The Astrophysical Journal. March 2009, 137 (3): 3558–3573. Bibcode:2009AJ....137.3558S. doi:10.1088/0004-6256/137/3/3558. 
  19. ^ Weaver, D.; Humphreys, R. Astronomers Map a Hypergiant Star's Massive Outbursts. HubbleSite NewsCenter. 2007-01-08 [2007-01-16]. （原始内容存档于2016-12-21）. 
  20. ^ Smartt, S. J.; Lennon, D. J.; Kudritzki, R. P.; Rosales, F.; Ryans, R. S. I.; Wright, N. The evolutionary status of Sher 25 - implications for blue supergiants and the progenitor of SN 1987A. Astronomy and Astrophysics. September 2002, 391: 979–991. Bibcode:2002A&A...391..979S. doi:10.1051/0004-6361:20020829. 
  21. ^ van Boekel, R.; Schöller, M.; Herbst, T. Biggest Star in Our Galaxy Sits within a Rugby-Ball Shaped Cocoon. European Organisation for Astronomical Research in the Southern Hemisphere (ESO). 2003-11-18 [2007-01-08]. （原始内容存档于2008-05-17）. 
  22. ^ Milan, Wil. Possible Hypernova Could Affect Earth. space.com. 2000-03-07 [2007-01-06]. （原始内容存档于2000-06-20）. 
  23. ^ Tuthill, Peter G.; et al.. The Prototype Colliding-Wind Pinwheel WR 104. The Astrophysical Journal. March 2008, 675 (1): 698–710. Bibcode:2008ApJ...675..698T. doi:10.1086/527286. 
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  25. ^ Jones, Terry Jay; et al.. IRC +10420 - A cool hypergiant near the top of the H-R diagram. Astrophysical Journal, Part 1. July 1993, 411 (1): 323–335. Bibcode:1993ApJ...411..323J. doi:10.1086/172832. 
  26. ^ Than, Ker. Astronomers Demonstrate a Global Internet Telescope. University of Manchester. 2004-10-04 [2007-01-08]. （原始内容存档于2008-05-05）. 
  27. ^ Staff. The William Herschel telescope finds the best candidate for a supernova explosion. Particle Physics and Astronomy Research Council. 2003-01-31 [2007-01-05]. （原始内容存档于2018-10-10）. 
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  29. ^ Woudt, P. A.; et al.. The Expanding Bipolar Shell of the Helium Nova V445 Puppis. The Astrophysical Journal. November 2009, 706 (1): 738–746. Bibcode:2009ApJ...706..738W. doi:10.1088/0004-637X/706/1/738. 
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  31. ^ Maxted, P. F. L.; Marsh, T. R.; North, R. C. KPD 1930+2752: a candidate Type Ia supernova progenitor. Monthly Notices of the Royal Astronomical Society. September 2000, 317 (3): L41–L44. Bibcode:2000MNRAS.317L..41M. doi:10.1046/j.1365-8711.2000.03856.x. 
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