Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

List of supernova candidates

From Wikipedia, the free encyclopedia

Map showing various supernova candidates, most of which are within one kiloparsec from the Solar System[1]

This is alist of supernova candidates, orstars that are believed to soon becomesupernovae.Type II supernova progenitors include stars with at least 8~10solar masses that are in the final stages of their evolution. Prominent examples of stars in this mass range includeAntares,Spica,Gamma Velorum,[2]Mu Cephei, and members of theQuintuplet Cluster.[3]Type Ia supernova progenitors arewhite dwarf stars that are close to theChandrasekhar limit of about 1.44 solar masses and are accreting matter from a binary companion star.

The list includes massiveWolf–Rayet stars, which may becomeType Ib/Ic supernovae, particularly oxygen-sequence (Wolf–Rayet WO) stars. As of 2023, most of these candidates are in theMilky Way galaxy; however, five oxygen-sequence Wolf–Rayet stars are also known in other galaxies.

Table

[edit]
This is adynamic list and may never be able to satisfy particular standards for completeness. You can help byediting the page to add missing items, with references toreliable sources.
IdentifierEpochJ2000ConstellationDistance

(light-years)

Spectral

class

Evolutionary stagePossible supernova

type

Notes
R. A.Dec.
Wolf 113020h 05m 19.5s[4]+54° 26′ 03″[4]Cygnus54.09±0.02[4]M3 + DMain sequence +white dwarfIa[5]
49 Librae16h 00m 19.61s[6]−16° 32′ 00.5″[6]Libra95.3±0.5F8V + DMain sequence +white dwarfIa[7]
NLTT 1275804h 12m 26.33s−11° 17′ 47.3″Eridanus[8]115±0.1D + DWhite dwarfIaSupernova will occur in 140 billion years[9]
IK Pegasi21h 26m 26.7s+19° 22′ 32″Pegasus154.4±1.0[10]A8m:/DAWhite dwarfIaSupernova will occur in 1.9 billion years[11]
WD J181058.67+311940.9418h 10m 58.7s+31° 19′ 40.9″Hercules[12]160D + DWhite dwarfIaSupernova will occur in 23 billion years[13]
Sigma Sagittarii (Nunki)18h 55m 15.93s–26° 17′ 48.2″Sagittarius228±5B2.5 VMain sequenceIISupernova will occur in over 20 million years[14]
Bellatrix (Gamma Orionis)05h 25m 07.86s+06° 20′ 58.9″Orion250±10B2 IIIBlue GiantII or Ia[15]
Spica (Alpha Virginis)13h 25m 11.6s−11° 09′ 40.8″Virgo250+14
−13
[16]
B1Subgiant[17]
Acrux (Alpha1 Crucis)12h 26m 35.9s–63° 05′ 56″Crux320±20[16]B0.5 IVMain sequence (blue dwarf)II[18]
Acrux (Alpha2 Crucis)12h 26m 36.4s–63° 05′ 58″Crux320±20[16]B1 VMain sequence (blue dwarf)II[18]
Zeta Ophiuchi16h 37m 09.5s−10° 34′ 02″Ophiuchus365±6.52[1]O9.5VMain sequence (blue dwarf)[1]
Betelgeuse (Alpha Orionis)05h 55m 10.3s+07° 24′ 25″Orion~400–500[19]M2IabRed supergiantIIP[20]
Alpha Lupi14h 41m 55.8s–47° 23′ 17″Lupus465+12
−11
[16]
B1.5Blue giantII[17]
Antares (Alpha Scorpii)16h 29m 24.5s–26° 25′ 55″Scorpius554+113
−80
[16]
M1.5Iab-bRed supergiantIIP[17]
Saiph (Kappa Orionis)05h 47m 45.38884s−09° 40′ 10.5777″Orion650 ± 30B0.5 IaBlue SupergiantII[21]
Pi Puppis (Ahadi)07h 17m 08.6s–37° 05′ 51″Puppis807+72
−61
[16]
K3 IbRed supergiantII?[1][22]
S Monocerotis A06h 40m 58.7s+09° 53′ 44″Monoceros920+150
−110
[16]
O7VMain sequence (blue dwarf)II[1]
S Monocerotis B06h 40m 58.7s+09° 53′ 44″Monoceros920+150
−110
[16]
O9.5VMain sequence (blue dwarf)II[1]
Rigel (Beta Orionis)05h 14m 32.3s–08° 12′ 06″Orion1,118+30
−28
[10]
B8IaBlue supergiantIIn(pec?)[23]
Gamma2 Velorum A08h 09m 32.0s−47° 20′ 12″Vela1,120+130
−100
[16]
WC8Wolf–Rayet starIb/Ic[24][2]
Gamma2 Velorum B08h 09m 32.0s−47° 20′ 12″Vela1,120+130
−100
[16]
O7.5IIIBlue supergiantII[25][2]
Mintaka Aa1 (Delta Orionis)05h 32m 00.4000s−00° 17′ 56.7424″Orion1,200O9.5IIBlue supergiantII[26]
Alnilam (Epsilon Orionis)05h 36m 12.81s−01° 12′ 06.9″Orion1,250±26B0 IaBlue supergiantII[27]
Alnitak Aa (Zeta Orionis)05h 40m 45.5s−01° 56′ 34.3″Orion1,260±180O9.5IabBlue supergiant[28]
HD 4979806h 48m 04.7s−44° 18′ 58″Puppis1,699±46[29]sdO5.5/D[30]White dwarfIaSupernova will occur in a few tens of thousands of years[31][32]
119 Tauri05h 32m 12.8s+18° 35′ 40″Taurus1,790+300
−220
[16]
M2Iab-IbRed supergiantIIb[1][22]
Deneb (Alpha Cygni)20h 41m 25.9s+45° 16′ 49″Cygnus2,615±215[1]A2laBlue supergiantIIL[1]
T Coronae Borealis15h 59m 30.2s+25° 55′ 13″Corona Borealis2,690+110
−100
[10]
M3III/DWhite dwarfIa[33]
KPD 1930+275219h 32m 14.9s+27° 58′ 35″Cygnus2,860+130
−120
[10]
sdB/DWhite dwarfIa[nb 1][34][35]
Mu Cephei21h 43m 30.5s+58° 46′ 48″Cepheus3,060+456
−130
[36]
M2IaRed hypergiantIIn/IIb[37]
Rho Cassiopeiae23h 54m 23.0s+57° 29′ 58″Cassiopeia3,440+930
−610
[10]
G2Ia0eYellow hypergiantIIL[38]
VY Canis Majoris07h 22m 58.3s−25° 46′ 03″Canis Major3,930+420
−350
[39]
M5eIaRed hypergiantII[20][40]
IRAS 17163-390717h 19m 49.3s−39° 10′ 37.9″Scorpius3,930+990
−660
[10]
late B/early AYellow hypergiantII[41]
Wray 17-9617h 41m 35.4s–30° 06′ 39″Scorpius3,940+1,110
−710
[10]
B3Luminous blue variable
VV Cephei A21h 56m 39.1s+63° 37′ 32″Cepheus4,900[42]M2IabRed hypergiant[1]
Mu Sagittarii18h 13m 14.8s–21° 03′ 32″Sagittarius5,100[43]B8IapBlue supergiant[44]
P Cygni20h 17m 47.2s+38° 01′ 59″Cygnus5,250±590[45]B1Ia+Luminous blue variableIIb[46]
HD 16862518h 21m 19.5s−16° 22′ 26″Sagittarius5,250+600
−490
[10]
B6IaLuminous blue variableII[47]
NML Cygni20h 46m 25.6s+40° 06′ 59.4″Cygnus5,250+420
−360
[48]
M6IRed hypergiantII[49]
IRC +1042019h 26m 48.1s+11° 21′ 17″Aquila5,600+2,200
−1,200
[10]
F8Ia+Yellow hypergiantIIb[50][51]
WR 14220h 21m 44.3s+37° 22′ 31″Cygnus5,670+290
−270
[10]
WO2Wolf–Rayet starIb/Ic
WR 13620h 12m 06.5s+38° 21′ 18″Cygnus6,700+500
−430
[10]
WN6(h)-sWolf–Rayet starIc
RS Ophiuchi17h 50m 13.2s–06° 42′ 28″Ophiuchus7,380+1,000
−790
[10]
M2III/DWhite dwarfIa
Eta Carinae10h 45m 03.6s−59° 41′ 04″Carina8,630+69
−68
[10]
LBV/OLuminous blue variableIb[52][53]
WR 93b17h 32m 03.3s−35° 04′ 32″Scorpius8,700+1,900
−1,300
[10]
WO3Wolf–Rayet starIb/Ic
WR 10217h 45m 47.5s−26° 10′ 27″Sagittarius9,410+840
−710
[10]
WO2Wolf–Rayet starIb/Ic
HD 17982119h 13m 58.6s+00° 07′ 32″Aquila10,500+2,100
−1,500
[10]
G5IaYellow hypergiantIIL[54][55]
T Pyxidis09h 04m 41.5s−32° 22′ 48″Pyxis10,700+1,700
−1,300
[10]
White dwarfIa[56][57]
WR 10418h 02m 04.1s–23° 37′ 41″Sagittarius13,400+9,200
−3,900
[10]
WC9d/OBWolf–Rayet starIb/Ic with Grb?[58][59]
AG Carinae10h 56m 11.57814s−60° 27′ 12.8107″Carina17,000±1,000LBV (WN11h-A-Ia)Luminous blue variableIIb[60]
WR 30a10h 51m 38.9s−60° 56′ 35.2″Carina38,900+18,500
−9,500
[10]
WO4/O5((f))Wolf–Rayet star
Sher 2511h 15m 07.8s−61° 15′ 17″Carina43,500+5,200
−4,200
[10]
B1.5IabBlue supergiant[61]
U Scorpii16h 22m 30.7s–17° 52′ 42″Scorpius63,900+68,500
−17,300
[62]
White dwarfIa[63]
LMC195-105h 18m 10.3s−69° 13′ 03″Dorado160,000[10]WO2Wolf–Rayet starIb/Ic
S Doradus05h 18m 14.4s−69° 15′ 01″Dorado169,000LBVLuminous blue variable[64]
SMC AB801h 31m 04.1s−73° 25′ 04″Hydrus200,000[10]WO4/O4Wolf–Rayet starIb/Ic
DR101h 05m 01.6s+02° 04′ 20″Cetus2,350,000WO3Wolf–Rayet starIb/Ic with Grb?[65]

Notes

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

References

[edit]
  1. ^abcdefghijMukhopadhyay, Mainak; Lunardini, Cecilia; Timmes, F. X.; Zuber, Kai (August 2020)."Presupernova Neutrinos: Directional Sensitivity and Prospects for Progenitor Identification".The Astrophysical Journal.899 (2): 153.arXiv:2004.02045.Bibcode:2020ApJ...899..153M.doi:10.3847/1538-4357/ab99a6.ISSN 0004-637X.
  2. ^abcKaler, James B."Regor".Stars.University of Illinois. Archived fromthe original on 2008-12-05. Retrieved2007-01-08.
  3. ^Lloyd, Robin (2006-09-04),Strange Space Pinwheels Spotted,space.com, retrieved2007-01-08
  4. ^abcVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  5. ^Mace, Gregory N.; Mann, Andrew W.; Skiff, Brian A.; Sneden, Christopher; Kirkpatrick, J. Davy; Schneider, Adam C.; Kidder, Benjamin; Gosnell, Natalie M.; Kim, Hwihyun; Mulligan, Brian W.; Prato, L.; Jaffe, Daniel (2018-02-01)."Wolf 1130: A Nearby Triple System Containing a Cool, Ultramassive White Dwarf".The Astrophysical Journal.854 (2): 145.arXiv:1802.04803.Bibcode:2018ApJ...854..145M.doi:10.3847/1538-4357/aaa8dd.ISSN 0004-637X.
  6. ^abBrown, 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. Gaia DR2 record for this source atVizieR.
  7. ^Fuhrmann, K.; Chini, R. (2017-01-02), "Bright Times for an Ancient Star",The Astrophysical Journal,834 (2): 114,Bibcode:2017ApJ...834..114F,doi:10.3847/1538-4357/834/2/114,S2CID 125888005.
  8. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  9. ^Kawka, Adela; Briggs, Gordon P.; Vennes, Stéphane; Ferrario, Lilia; Paunzen, Ernst; Wickramasinghe, Dayal T. (2016-12-05)."A fast spinning magnetic white dwarf in the double degenerate, super-Chandrasekhar system NLTT 12758".Monthly Notices of the Royal Astronomical Society.466 (1):1127–1139.arXiv:1612.00325.doi:10.1093/mnras/stw3149.ISSN 0035-8711.
  10. ^abcdefghijklmnopqrstuvBrown, 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.
  11. ^Beech, Martin (2011-12-01)."The past, present and future supernova threat to Earth's biosphere".Astrophysics and Space Science.336:287–302.doi:10.1007/s10509-011-0873-9.ISSN 0004-640X.
  12. ^Roman, Nancy G. (1987)."Identification of a constellation from a position".Publications of the Astronomical Society of the Pacific.99 (617): 695.Bibcode:1987PASP...99..695R.doi:10.1086/132034. Constellation record for this object atVizieR.
  13. ^Munday, James; Pakmor, Ruediger; Pelisoli, Ingrid; Jones, David; Sahu, Snehalata; Tremblay, Pier-Emmanuel; Rajamuthukumar, Abinaya Swaruba; Nelemans, Gijs; Magee, Mark (2025-04-06). "A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr".Nature Astronomy.arXiv:2504.04522.doi:10.1038/s41550-025-02528-4.
  14. ^Waisberg, Idel; Klein, Ygal; Katz, Boaz (April 2025)."Hidden Companions to Intermediate-mass Stars. XXVI. Uncovering Nunki = Sigma Sagittarii as a 6.5 M⊙ + 6.3 M⊙, 0.60 au Binary".Research Notes of the AAS.9 (4): 71.doi:10.3847/2515-5172/adc739.
  15. ^Kaler, James B."BELLATRIX (Gamma Orionis)".Stars. University of Illinois. Retrieved2012-12-27.
  16. ^abcdefghijkvan Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entry
  17. ^abcFirestone, 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.
  18. ^ab"Acrux (Alpha Crucis)". illinois.edu. Retrieved2020-11-20.
  19. ^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.
  20. ^abSmith, 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.
  21. ^"Saif".stars.astro.illinois.edu. Retrieved2025-09-13.
  22. ^abAsakura, 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.
  23. ^Moravveji, Ehsan; Guinan, Edward F.; Shultz, Matt; Williamson, Michael H.; Moya, Andres (March 2012), "Asteroseismology of the nearby SN-II Progenitor: Rigel. Part I. TheMOST 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
  24. ^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
  25. ^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
  26. ^"Mintaka".stars.astro.illinois.edu. Retrieved2025-09-18.
  27. ^"Alnilam".stars.astro.illinois.edu. Retrieved2025-09-18.
  28. ^Berman, Bob (2023-04-10)."Alnitak: an exceptionally hot, blue star on Orion's Belt | Astronomy.com".Astronomy Magazine. Retrieved2024-09-02.
  29. ^Rigoselli, Michela; De Grandis, Davide; Mereghetti, Sandro; Malacaria, Christian (30 May 2023)."Timing the X-ray pulsating companion of the hot subdwarf HD 49798 with NICER".Monthly Notices of the Royal Astronomical Society.523 (2):3043–3048.arXiv:2305.15845.doi:10.1093/mnras/stad1611.
  30. ^Mereghetti, S.; Tiengo, A.; Esposito, P.; La Palombara, N.; Israel, G. L.; Stella, L. (2009). "An Ultramassive, Fast-Spinning White Dwarf in a Peculiar Binary System".Science.325 (5945):1222–1223.arXiv:1003.0997.Bibcode:2009Sci...325.1222M.doi:10.1126/science.1176252.PMID 19729650.S2CID 206521141.
  31. ^Wang, Bo; Han, Zhanwen (2012). "Progenitors of type Ia supernovae".New Astronomy Reviews.56 (4): 122.arXiv:1204.1155.Bibcode:2012NewAR..56..122W.doi:10.1016/j.newar.2012.04.001.S2CID 118740933.
  32. ^Liu, Dong-Dong; Zhou, Wei-Hong; Wu, Cheng-Yuan; Wang, Bo (2015). "Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor?".Research in Astronomy and Astrophysics.15 (11): 1813.arXiv:1504.01461.Bibcode:2015RAA....15.1813L.doi:10.1088/1674-4527/15/11/004.S2CID 118683249.
  33. ^"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. Retrieved2013-01-03.
  34. ^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.
  35. ^Kanipe, Jeff (2000-08-05)."Skywatch—Watch This Space!".space.com. Archived fromthe original on 2009-07-20. Retrieved2007-01-06.
  36. ^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.
  37. ^Lloyd, Robin (2006-09-04)."Strange Space Pinwheels Spotted".space.com. Retrieved2007-01-08.
  38. ^"The William Herschel telescope finds the best candidate for a supernova explosion". Particle Physics and Astronomy Research Council. 2003-01-31. Retrieved2007-01-05.
  39. ^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.
  40. ^Weaver, Donna; Humphreys, Roberta (2007-01-08)."Astronomers Map a Hypergiant Star's Massive Outbursts".HubbleSite NewsCenter. Archived fromthe original on 2007-01-12. Retrieved2007-01-16.
  41. ^"'Fried Egg' Nebula Cracks Open Rare Hypergiant Star". Space.com. 2011-09-28. Retrieved2015-06-13.
  42. ^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.
  43. ^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.
  44. ^"Polis".stars.astro.illinois.edu. Retrieved2024-10-18.
  45. ^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.
  46. ^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.
  47. ^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.
  48. ^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.
  49. ^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.
  50. ^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.
  51. ^Than, Ker (2004-10-04)."Astronomers Demonstrate a Global Internet Telescope". University of Manchester. Retrieved2007-01-08.
  52. ^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 fromthe original on 2007-01-03. Retrieved2007-01-08.
  53. ^Milan, Wil (2000-03-07)."Possible Hypernova Could Affect Earth".space.com. Retrieved2007-01-06.
  54. ^Jura, M.; Velusamy, T.; Werner, M. W. (2001-06-05)."What next for the Likely Pre-Supernova, HD 179821?".American Astronomical Society. Archived fromthe original on 2008-07-08. Retrieved2007-01-08.
  55. ^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.
  56. ^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.
  57. ^Edwards, Lin (2010)."Massive white dwarf in our galaxy may go supernova".PhysOrg. Retrieved2010-02-26.
  58. ^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.
  59. ^Kaler, Jim (1999-04-09)."WR 104: Pinwheel Star".Astronomy Picture of the Day. Archived fromthe original on 2009-04-14. Retrieved2007-01-08.
  60. ^Groh, J. H.; Meynet, G.; Ekström, S. (2013). "Massive star evolution: luminous blue variables as unexpected supernova progenitors".Astronomy & Astrophysics.550: 4.arXiv:1301.1519.Bibcode:2013A&A...550L...7G.doi:10.1051/0004-6361/201220741.S2CID 119227339. L7.
  61. ^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.
  62. ^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.
  63. ^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.
  64. ^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.
  65. ^Tramper, F.; Gräfener, G.; Hartoog, O. E.; Sana, H.; de Koter, A.; Vink, J. S.; Ellerbroek, L. E.; Langer, N.; Garcia, M.; Kaper, L.; de Mink, S. E. (2013)."On the nature of WO stars: a quantitative analysis of the WO3 star DR1 in IC 1613".Astronomy & Astrophysics.559: A72.arXiv:1310.2849.Bibcode:2013A&A...559A..72T.doi:10.1051/0004-6361/201322155.ISSN 0004-6361.
Retrieved from "https://en.wikipedia.org/w/index.php?title=List_of_supernova_candidates&oldid=1316412144"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp