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超新星候选列表

维基百科，自由的百科全书

超新星候选列表是天文学家提出将成为超新星前身的恒星。II型超新星的前身包括演化至最后阶段的质量仍然大于10倍太阳质量的恒星(在这个质量范围内的恒星，著名的例子包括心宿二、角宿一[1]、天社一[2] 仙王座μ和五合星团中的一些成员[3]。)。Ia型超新星的前身是接近钱德拉塞卡极限，经由伴星吸积至大约是1.44太阳质量的白矮星。这张表也包括大质量的沃夫-瑞叶星，它们可能会成为Ia/Ib超新星。

 本表是动态列表，或许永远不会完结。欢迎您参考可靠来源来查漏补缺。
超新星前身候选者
名称 历元 J2000 星座 距离
(光年) 		光谱
分类 		注解
R. A. Dec.
飞马座IK 21h 26m 26.7s +19° 22′ 32″ 飞马座 150 A8m:/DA [4][5]
角宿一 13h 25m 11.6s -11° 09′ 40.8″ 室女座 250 B1 [6]
骑官十 14h 41m 56s –47° 23′ 17″ 豺狼座 550 B1.5 [7][6]
心宿二 16h 29m 24s –26° 25′ 55″ 天蝎座 600 M1.5Iab-b [8][6]
参宿四 05h 55m 10.3s +07° 24′ 25″ 猎户座 640 M2Iab [1][9]
天社一 08h 09m 32.0s −47° 20′ 12″ 船帆座 800 WC8 [9]
参宿七 05h 14m 32.3s –08° 12′ 06″ 猎户座 860 B8Ia [10][6]
弧矢九 7h 17m 08s –37° 05′ 51″ 船尾座 1,100 K3 Ib
金牛座119 05h 32m 12.8s +18° 35′ 40″ 金牛座 1,700 M2Iab-Ib
蛇夫座RS 17h 50m 13.2s –06° 42′ 28″ 蛇夫座 1,950–5,200 M2III/D [11][12]
HD 168625 18h 21m 19.5s −16° 22′ 26″ 人马座 7,200 B6Ia [13]
罗盘座T 09h 04m 41.5s −32° 22′ 48″ 罗盘座 3,260 [14][15]
HD 179821 19h 13m 58.6s +00° 07′ 32″ 天鹰座 3,300 G5Ia [16][17]
大犬座VY 07h 22m 58.3s −25° 46′ 03″ 大犬座 4,900 M5eIa [18][19]
Sher 25 11h 15m 07.8s −61° 15′ 17″ 船底座 ~20,000 B1.5Iab [20]
海山二 10h 45m 03.6s −59° 41′ 04″ 船底座 7,000–8,000 B3-5Ia0/O7I(WC8) [21][22]
WR 104 18h 02m 04.1s –23° 37′ 41″ 人马座 8,000 WC9d/OB [23][24]
IRC+10420 19h 26m 48.1s +11° 21′ 17″ 天鹰座 10,000-23,000 F8Ia+ [25][26]
仙后座ρ 23h 54m 23.0s +57° 29′ 58″ 仙后座 12,000 G2Ia0e [27]
HD 179821 19h 13m 58.6s +00° 07′ 32″ 天鹰座 20,000 G5Ia [17][28]
船尾座V445 07h 37m 56.9s –25° 56′ 59″ 船尾座 27,000 [29]
天蝎座U 16h 22m 30.7s –17° 52′ 42″ 天蝎座 39,000 [30]
KPD1930+2752 19h 32m 14.9s +27° 58′ 35″ 天鹅座 sdB/D [nb 1][31][32]

注解

[编辑]
  1. ^ The Kitt Peak Downes star.

参考资料

[编辑]
  1. ^ 1.0 1.1 Supernova Remnants and Neutron Stars. Harvard-Smithsonian Center for Astrophysics. 2005-08-02 [2006-06-08]. （原始内容存档于2015-06-12）. 
  2. ^ Kaler, Jim. Regor. University of Illinois. [2007-01-08]. （原始内容存档于2008-12-05）. 
  3. ^ Lloyd, Robin. Strange Space Pinwheels Spotted. space.com. 2006-09-04 [2007-01-08]. （原始内容存档于2010-08-29）. 
  4. ^ Samuel, Eugenie. Supernova poised to go off near Earth. New Scientist. 2002-05-23 [2007-01-12]. （原始内容存档于2008-09-15）. 
  5. ^ Tzekova, S. Y.; et al. IK Pegasi (HR 8210). ESO. 2004 [2007-01-12]. （原始内容存档于2020-05-26）. 
  6. ^ 6.0 6.1 6.2 6.3 Firestone, R. B., Observation of 23 Supernovae That Exploded <300 pc from Earth during the past 300 kyr, The Astrophysical Journal, July 2014, 789 (1): 11, Bibcode:2014ApJ...789...29F, doi:10.1088/0004-637X/789/1/29, 29.  See Table 4, p. 10.
  7. ^ Big and Giant Stars: Alpha Lupi. Jumk.de. [2013-01-03]. （原始内容存档于2019-12-15）. 
  8. ^ What will happen when Antares explodes?. Disassociated.com. 2009-01-13 [2013-01-03]. （原始内容存档于2018-11-18）. 
  9. ^ 9.0 9.1 Beech, Martin, The past, present and future supernova threat to Earth's biosphere, Astrophysics and Space Science, December 2011, 336 (2): 287–302, Bibcode:2011Ap&SS.336..287B, doi:10.1007/s10509-011-0873-9 
  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 可免费查阅, 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）. 
  16. ^ 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]. （原始内容存档于2008-07-08）. 
  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. 
  24. ^ Kaler, Jim. WR 104: Pinwheel Star. Astronomy Picture of the Day. 1999-04-09 [2007-01-08]. （原始内容存档于2009-04-14）. 
  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）. 
  28. ^ 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]. （原始内容存档于2008-07-08）. 
  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. 
  30. ^ 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. 
  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. 
  32. ^ Kanipe, Jeff. Skywatch—Watch This Space!. space.com. 2000-08-05 [2007-01-06]. （原始内容存档于2009-07-20）. 
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