Map showing various supernova candidates, most of which are within one kiloparsec from the Solar System.[ 1]
This is a list of supernova candidates , or stars that are believed to soon become supernovae . Type II supernova progenitors include stars with at least 8~10 solar masses that are in the final stages of their evolution. Prominent examples of stars in this mass range include Antares , Spica , Gamma Velorum ,[ 2] Mu Cephei , and members of the Quintuplet Cluster .[ 3] Type Ia supernova progenitors are white dwarf stars that are close to the Chandrasekhar limit of about 1.44 solar masses and are accreting matter from a binary companion star.
The list includes massive Wolf–Rayet stars , which may become Type Ib/Ic supernovae , particularly oxygen-sequence (Wolf-Rayet WO) stars. As of 2023, most of these candidates are in the Milky Way galaxy, however five oxygen-sequence Wolf-Rayet stars are also known in other galaxies.
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^ a b c d e f g h i j k l m n o p q r s t u v Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 .
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^ a b c Firestone, R. B. (July 2014), "Observation of 23 Supernovae That Exploded <300 pc from Earth during the past 300 kyr" , The Astrophysical Journal , 789 (1): 11, Bibcode :2014ApJ...789...29F , doi :10.1088/0004-637X/789/1/29 , 29. See Table 4, p. 10.
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^ Neuhäuser, Ralph; Torres, Guillermo; Mugrauer, Markus; Neuhäuser, Dagmar L.; Chapman, Jesse; Luge, Daniela; Cosci, Matteo (2022-09-05). "Colour evolution of Betelgeuse and Antares over two millennia, derived from historical records, as a new constraint on mass and age" . Monthly Notices of the Royal Astronomical Society . 516 (1): 693–719. arXiv :2207.04702 . doi :10.1093/mnras/stac1969 . ISSN 0035-8711 .
^ a b Smith, Nathan; Hinkle, Kenneth H.; Ryde, Nils (2009-03-01). "Red Supergiants as Potential Type IIn Supernova Progenitors: Spatially Resolved 4.6 μm CO Emission Around VY CMa and Betelgeuse". The Astronomical Journal . 137 (3): 3558–3573. arXiv :0811.3037 . Bibcode :2009AJ....137.3558S . doi :10.1088/0004-6256/137/3/3558 . ISSN 0004-6256 . S2CID 19019913 .
^ a b Asakura, K.; Gando, A.; Gando, Y.; Hachiya, T.; Hayashida, S.; Ikeda, H.; Inoue, K.; Ishidoshiro, K.; Ishikawa, T.; Ishio, S.; Koga, M.; Matsuda, S.; Mitsui, T.; Motoki, D.; Nakamura, K. (February 2016). "KamLAND SENSITIVITY TO NEUTRINOS FROM PRE-SUPERNOVA STARS" . The Astrophysical Journal . 818 (1): 91. arXiv :1506.01175 . Bibcode :2016ApJ...818...91A . doi :10.3847/0004-637X/818/1/91 . ISSN 0004-637X .
^ Moravveji, Ehsan; Guinan, Edward F.; Shultz, Matt; Williamson, Michael H.; Moya, Andres (March 2012), "Asteroseismology of the nearby SN-II Progenitor: Rigel. Part I. The MOST High-precision Photometry and Radial Velocity Monitoring", The Astrophysical Journal , 747 (1): 108–115, arXiv :1201.0843 , Bibcode :2012ApJ...747..108M , doi :10.1088/0004-637X/747/2/108 , S2CID 425831
^ Thielemann, Friedrich-Karl; Hirschi, Raphael; Liebendörfer, Matthias; Diehl, Roland (2011), "Massive Stars and their Supernovae", Astronomy with Radioactivities , Lecture Notes in Physics, vol. 812, pp. 153–231, arXiv :1008.2144 , Bibcode :2011LNP...812..153T , doi :10.1007/978-3-642-12698-7_4 , ISBN 978-3-642-12697-0
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^ "Recurrent Novae as a Progenitor System of Type Ia Supernovae. I. RS Ophiuchi Subclass: Systems with a Red Giant Companion - Abstract - The Astrophysical Journal - IOPscience" . Iopscience.iop.org. 2008-12-19. Retrieved 2013-01-03 .
^ Maxted, P. F. L.; Marsh, T. R.; North, R. C. (2000-09-21). "KPD 1930+2752: a candidate Type Ia supernova progenitor" . Monthly Notices of the Royal Astronomical Society . 317 (3): L41–L44. arXiv :astro-ph/0007257 . Bibcode :2000MNRAS.317L..41M . doi :10.1046/j.1365-8711.2000.03856.x . ISSN 0035-8711 . S2CID 11267384 .
^ Kanipe, Jeff (2000-08-05). "Skywatch—Watch This Space!" . space.com . Archived from the original on 2009-07-20. Retrieved 2007-01-06 .
^ Davies, Ben; Beasor, Emma R (2020-01-20). "The 'red supergiant problem': the upper luminosity boundary of Type II supernova progenitors" . Monthly Notices of the Royal Astronomical Society . 493 (1): 468–476. arXiv :2001.06020 . doi :10.1093/mnras/staa174 . ISSN 0035-8711 .
^ Lloyd, Robin (2006-09-04). "Strange Space Pinwheels Spotted" . space.com . Retrieved 2007-01-08 .
^ "The William Herschel telescope finds the best candidate for a supernova explosion" . Particle Physics and Astronomy Research Council. 2003-01-31. Retrieved 2007-01-05 .
^ Zhang, B.; Reid, M. J.; Menten, K. M.; Zheng, X. W. (January 2012). "Distance and Kinematics of the Red Hypergiant VY CMa: VLBA and VLA Astrometry". The Astrophysical Journal . 744 (1): 23. arXiv :1109.3036 . Bibcode :2012ApJ...744...23Z . doi :10.1088/0004-637X/744/1/23 .
^ Weaver, Donna; Humphreys, Roberta (2007-01-08). "Astronomers Map a Hypergiant Star's Massive Outbursts" . HubbleSite NewsCenter . Archived from the original on 2007-01-12. Retrieved 2007-01-16 .
^ " 'Fried Egg' Nebula Cracks Open Rare Hypergiant Star" . Space.com. 2011-09-28. Retrieved 2015-06-13 .
^ Bauer, Wendy Hagen; Gull, Theodore R.; Bennett, Philip D. (2008-09-01). "Spatial Extension in the Ultraviolet Spectrum of Vv Cephei". The Astronomical Journal . 136 (3): 1312–1324. Bibcode :2008AJ....136.1312H . doi :10.1088/0004-6256/136/3/1312 . ISSN 0004-6256 .
^ Gaia Collaboration; Vallenari, A.; Brown, A. G. A.; Prusti, T.; de Bruijne, J. H. J.; Arenou, F.; Babusiaux, C.; Biermann, M.; Creevey, O. L.; Ducourant, C.; Evans, D. W.; Eyer, L.; Guerra, R.; Hutton, A.; Jordi, C. (June 2023). "Gaia Data Release 3: Summary of the content and survey properties". Astronomy & Astrophysics . 674 : A1. arXiv :2208.00211 . Bibcode :2023A&A...674A...1G . doi :10.1051/0004-6361/202243940 . ISSN 0004-6361 .
^ "Polis" . stars.astro.illinois.edu . Retrieved 2024-10-18 .
^ de Almeida, E S G; Hugbart, M; Domiciano de Souza, A; Rivet, J-P; Vakili, F; Siciak, A; Labeyrie, G; Garde, O; Matthews, N; Lai, O; Vernet, D; Kaiser, R; Guerin, W (2022-06-15). "Combined spectroscopy and intensity interferometry to determine the distances of the blue supergiants P Cygni and Rigel" . Monthly Notices of the Royal Astronomical Society . 515 (1): 1–12. arXiv :2204.00372 . doi :10.1093/mnras/stac1617 . ISSN 0035-8711 .
^ Groh, Jose H.; Meynet, Georges; Ekström, Sylvia (February 2013). "Massive star evolution: Luminous Blue Variables as unexpected Supernova progenitors". Astronomy & Astrophysics . 550 : L7. arXiv :1301.1519 . Bibcode :2013A&A...550L...7G . doi :10.1051/0004-6361/201220741 . ISSN 0004-6361 .
^ Smith, Nathan (March 2007). "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 . 133 (3): 1034–1040. arXiv :astro-ph/0611544 . Bibcode :2007AJ....133.1034S . doi :10.1086/510838 . S2CID 17598600 .
^ Zhang, B.; Reid, M. J.; Menten, K. M.; Zheng, X. W.; Brunthaler, A. (2012). "The distance and size of the red hypergiant NML Cygni from VLBA and VLA astrometry" (PDF) . Astronomy & Astrophysics . 544 : A42. arXiv :1207.1850 . Bibcode :2012A&A...544A..42Z . doi :10.1051/0004-6361/201219587 . S2CID 55509287 .
^ Monnier, J. D.; Millan-Gabet, R.; Tuthill, P. G.; Traub, W. A.; Carleton, N. P.; Coude Du Foresto, V.; Danchi, W. C.; Lacasse, M. G.; Morel, S.; Perrin, G.; Porro, I. L.; Schloerb, F. P.; Townes, C. H. (2004). "High-Resolution Imaging of Dust Shells by Using Keck Aperture Masking and the IOTA Interferometer". The Astrophysical Journal . 605 (1): 436–461. arXiv :astro-ph/0401363 . Bibcode :2004ApJ...605..436M . doi :10.1086/382218 . S2CID 7851916 .
^ Jones, Terry Jay; et al. (July 1993). "IRC +10420 - A cool hypergiant near the top of the H-R diagram". The Astrophysical Journal . 411 (1): 323. Bibcode :1993ApJ...411..323J . doi :10.1086/172832 . ISSN 0004-637X .
^ Than, Ker (2004-10-04). "Astronomers Demonstrate a Global Internet Telescope" . University of Manchester. Retrieved 2007-01-08 .
^ van Boekel, Roy; Schöller, Markus; Herbst, Tom (2003-11-18). "Biggest Star in Our Galaxy Sits within a Rugby-Ball Shaped Cocoon" . European Southern Observatory Press Release . European Organisation for Astronomical Research in the Southern Hemisphere (ESO): 31. Bibcode :2003eso..pres...36. Archived from the original on 2007-01-03. Retrieved 2007-01-08 .
^ Milan, Wil (2000-03-07). "Possible Hypernova Could Affect Earth" . space.com . Retrieved 2007-01-06 .
^ Jura, M.; Velusamy, T.; Werner, M. W. (2001-06-05). "What next for the Likely Pre-Supernova, HD 179821?" . American Astronomical Society . Archived from the original on 2008-07-08. Retrieved 2007-01-08 .
^ Josselin, E.; Lèbre, A. (March 2001). "Probing the post-AGB nature of HD 179821: A new radio study of its circumstellar envelope" . Astronomy & Astrophysics . 367 (3): 826–830. Bibcode :2001A&A...367..826J . doi :10.1051/0004-6361:20000496 . ISSN 0004-6361 .
^ Schaefer, Bradley E.; Pagnotta, Ashley; Shara, Michael M. (2010-01-01). "The Nova Shell and Evolution of the Recurrent Nova T Pyxidis". The Astrophysical Journal . 708 (1): 381–402. arXiv :0906.0933 . Bibcode :2010ApJ...708..381S . doi :10.1088/0004-637X/708/1/381 . ISSN 0004-637X . S2CID 18807684 .
^ Edwards, Lin (2010). "Massive white dwarf in our galaxy may go supernova" . PhysOrg . Retrieved 2010-02-26 .
^ Tuthill, Peter G.; et al. (March 2008). "The Prototype Colliding-Wind Pinwheel WR 104". The Astrophysical Journal . 675 (1): 698–710. arXiv :0712.2111 . Bibcode :2008ApJ...675..698T . doi :10.1086/527286 . ISSN 0004-637X . S2CID 119293391 .
^ Kaler, Jim (1999-04-09). "WR 104: Pinwheel Star" . Astronomy Picture of the Day . Archived from the original on 2009-04-14. Retrieved 2007-01-08 .
^ Kato, Mariko; Hachisu, Izumi; Kiyota, Seiichiro; Saio, Hideyuki (2008-09-10). "Helium Nova on a Very Massive White Dwarf: A Revised Light-Curve Model of V445 Puppis (2000)". The Astrophysical Journal . 684 (2): 1366–1373. arXiv :0805.2540 . Bibcode :2008ApJ...684.1366K . doi :10.1086/590329 . ISSN 0004-637X . S2CID 18001230 .
^ Woudt, P. A.; et al. (2009-11-20). "The Expanding Bipolar Shell of the Helium Nova V445 Puppis". The Astrophysical Journal . 706 (1): 738–746. arXiv :0910.1069 . Bibcode :2009ApJ...706..738W . doi :10.1088/0004-637X/706/1/738 . ISSN 0004-637X . S2CID 85461691 .
^ Smartt, S. J.; Lennon, D. J.; Kudritzki, R. P.; Rosales, F.; Ryans, R. S. I.; Wright, N. (September 2002). "The evolutionary status of Sher 25 – implications for blue supergiants and the progenitor of SN 1987A". Astronomy & Astrophysics . 391 (3): 979–991. arXiv :astro-ph/0205242 . Bibcode :2002A&A...391..979S . doi :10.1051/0004-6361:20020829 . ISSN 0004-6361 . S2CID 14933392 .
^ Schaefer, Bradley E. (2018-09-01). "The distances to Novae as seen by Gaia" . Monthly Notices of the Royal Astronomical Society . 481 (3): 3033–3051. arXiv :1809.00180 . doi :10.1093/mnras/sty2388 .
^ Thoroughgood, T. D.; Dhillon, V. S.; Littlefair, S. P.; Marsh, T. R.; Smith, D. A. (2001). "The Recurrent Nova U Scorpii - A Type Ia Supernova Progenitor". The Physics of Cataclysmic Variables and Related Objects . Vol. 261. San Francisco, CA: Astronomical Society of the Pacific. arXiv :astro-ph/0109553 . Bibcode :2002ASPC..261...77T .
^ Kalari, V. M.; Vink, J. S.; Dufton, P. L.; Fraser, M. (2018-10-01). "How common is LBV S Doradus variability at low metallicity?" . Astronomy & Astrophysics . 618 : A17. arXiv :1807.01309 . Bibcode :2018A&A...618A..17K . doi :10.1051/0004-6361/201833484 . ISSN 0004-6361 .
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