超新星候選列表

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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卓極限，經由伴星吸積至大約是1.38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。

Nuvola apps kalarm.png这是一個动态的未完成列表，内容可能会随时发生变动，所以它可能永远也不会補充完整，但歡迎您隨時修改并列明来源。
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IK 21h 26m 26.7s +19° 22′ 32″ 飛馬座 150 A8m:/DA [4][5]
参宿四 05h 55m 10.3s +07° 24′ 25″ 獵戶座 640 M2Iab [1][6]
蛇夫座RS 17h 50m 13.2s –06° 42′ 28″ 蛇夫座 1,950–5,200 M2III/D [7][8]
HD 168625 18h 21m 19.5s −16° 22′ 26″ 人馬座 2,200 B6Ia [9]
羅盤座T 09h 04m 41.5s −32° 22′ 48″ 羅盤座 3,260 [10][11]
HD 179821 19h 13m 58.6s +00° 07′ 32″ 天鷹座 3,300 G5Ia [12][13]
大犬座VY 07h 22m 58.3s −25° 46′ 03″ 大犬座 4,900 M5eIa [6][14]
Sher 25 11h 15m 07.8s −61° 15′ 17″ 船底座 ~20,000 B1.5Iab [15]
海山二 10h 45m 03.6s −59° 41′ 04″ 船底座 7,000–8,000 Wolf-rayet [16][17]
WR 104 18h 02m 04.1s –23° 37′ 41″ 人馬座 8,000 WC9d/OB [18][19]
IRC+10420 19h 26m 48.1s +11° 21′ 17″ 天鷹座 10,000-23,000 F8Ia+ [20][21]
仙后座ρ 23h 54m 23.0s +57° 29′ 58″ 仙后座 12,000 G2Ia0e [22]
HD 179821 19h 13m 58.6s +00° 07′ 32″ 天鷹座 20,000 G5Ia [13][23]
船尾座V445 07h 37m 56.9s –25° 56′ 59″ 船尾座 27,000 [24]
天蝎座U 16h 22m 30.7s –17° 52′ 42″ 天蝎座 39,000 [25]
KPD1930+2752 19h 32m 14.9s +27° 58′ 35″ 天鵝座 sdB/D [nb 1][26][27]

註解 [编辑]

  1. ^ The Kitt Peak Downes star.

參考資料 [编辑]

  1. ^ 1.0 1.1 Supernova Remnants and Neutron Stars. Harvard-Smithsonian Center for Astrophysics. 2005-08-02 [2006-06-08]. 
  2. ^ Kaler, Jim. Regor. University of Illinois. [2007-01-08]. 
  3. ^ Lloyd, Robin. Strange Space Pinwheels Spotted. space.com. 2006-09-04 [2007-01-08]. 
  4. ^ Samuel, Eugenie. Supernova poised to go off near Earth. New Scientist. 2002-05-23 [2007-01-12]. 
  5. ^ Tzekova, S. Y. et al.. IK Pegasi (HR 8210). ESO. 2004 [2007-01-12]. 
  6. ^ 6.0 6.1 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. 2009.March, 137 (3): 3558–3573. Bibcode:2009AJ....137.3558S. doi:10.1088/0004-6256/137/3/3558. 
  7. ^ Than, Ker. Mystery of Explosive Star Solved. space.com. 2006-07-19 [2007-01-08]. 
  8. ^ Staff. Astronomers See Future Supernova Developing. SpaceDaily. 2006-07-25 [2006-12-01]. 
  9. ^ 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. 2007.March, (3): 1034–1040. Bibcode:2007AJ....133.1034S. doi:10.1086/510838.  已忽略文本“ volume 133 ” (帮助)
  10. ^ Schaefer, Bradley E.; Pagnotta, Ashley; Shara, Michael M. The Nova Shell and Evolution of the Recurrent Nova T Pyxidis. 2010.January. Bibcode:2010ApJ...708..381S. doi:10.1088/0004-637X/708/1/381. 
  11. ^ Edwards, Lin. Massive white dwarf in our galaxy may go supernova. PhysOrg. 2010 [2010-02-26]. 
  12. ^ Jura, M.; Velusamy, T.; Werner, M. W. What next for the Likely Pre-Supernova, HD 179821?. American Astronomical Society. 2001-06-05 [2007-01-08]. 
  13. ^ 13.0 13.1 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. 
  14. ^ Weaver, D.; Humphreys, R. Astronomers Map a Hypergiant Star's Massive Outbursts. HubbleSite NewsCenter. 2007-01-08 [2007-01-16]. 
  15. ^ 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. 2002.September, 391: 979–991. Bibcode:2002A&A...391..979S. doi:10.1051/0004-6361:20020829. 
  16. ^ 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]. 
  17. ^ Milan, Wil. Possible Hypernova Could Affect Earth. space.com. 2000-03-07 [2007-01-06]. 
  18. ^ Tuthill, Peter G.; et al.. The Prototype Colliding-Wind Pinwheel WR 104. The Astrophysical Journal. 2008.March, 675 (1): 698–710. Bibcode:2008ApJ...675..698T. doi:10.1086/527286. 
  19. ^ Kaler, Jim. WR 104: Pinwheel Star. Astronomy Picture of the Day. 1999-04-09 [2007-01-08]. 
  20. ^ Jones, Terry Jay; et al.. IRC +10420 - A cool hypergiant near the top of the H-R diagram. Astrophysical Journal, Part 1. 1993.July, 411 (1): 323–335. Bibcode:1993ApJ...411..323J. doi:10.1086/172832. 
  21. ^ Than, Ker. Astronomers Demonstrate a Global Internet Telescope. University of Manchester. 2004-10-04 [2007-01-08]. 
  22. ^ 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]. 
  23. ^ Jura, M.; Velusamy, T.; Werner, M. W. What next for the Likely Pre-Supernova, HD 179821?. American Astronomical Society. 2001-06-05 [2007-01-08]. 
  24. ^ Woudt, P. A.; et al.. The Expanding Bipolar Shell of the Helium Nova V445 Puppis. The Astrophysical Journal. 2009.November, 706 (1): 738–746. Bibcode:2009ApJ...706..738W. doi:10.1088/0004-637X/706/1/738. 
  25. ^ Thoroughgood, T. D.; Dhillon, V. S.; Littlefair, S. P.; Marsh, T. R.; Smith, D. A.. The recurrent nova U Scorpii -- A type Ia supernova progenitor. The Physics of Cataclysmic Variables and Related Objects, 261. San Francisco, CA: Astronomical Society of the Pacific. 2002 [2009-01-24]. Bibcode 2002ASPC..261...77T. 
  26. ^ 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. 2000.September, 317 (3): L41–L44. Bibcode:2000MNRAS.317L..41M. doi:10.1046/j.1365-8711.2000.03856.x. 
  27. ^ Kanipe, Jeff. Skywatch—Watch This Space!. space.com. 2000-08-05 [2007-01-06]. 
分類
相關的
結構
前身
殘骸
發現
列表
著名的
研究
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