Movatterモバイル変換

[0]ホーム
URL:

Jump to content
WikipediaThe Free Encyclopedia
Search

List of supernovae

From Wikipedia, the free encyclopedia

SN 1054 remnant
(Crab Nebula)

Asupernova is an event in which astar destroys itself in an explosion which can briefly become as luminous as an entiregalaxy. Thislist of supernovas of historical significance includes events that were observed prior to the development of photography, and individual events that have been the subject of a scientific paper that contributed to supernova theory.

List of supernovae

[edit]

In most entries, the year when the supernova was seen is part of the designation (1st column).

Supernova
designation
(year)		ConstellationObservationsApparent
magnitude		Distance
(light years)		TypeGalaxyNotes
SN 185Centaurus7 December 185−4 (?)[1]9,100[2]Ia (?)Milky WaySurviving description sketchy; modern estimates of maximum apparent magnitude vary from +4 to −8. The remnant is probablyRCW 86, some 8200 ly distant,[3] making it comparable toSN 1572. Some researchers have suggested it was a comet, not a supernova.[4][5]
SN 386SagittariusApril/May 386+1.514,700IIMilky Way"suggested SN",[6] candidate remnant could be G11.2-0.3.[7][8] There are three suggestions and doubtful if SN at all or classical nova or something else.[9]
SN 393Scorpius27 February − 28 March - 22 October − 19 November 393–03,400 II/IbMilky Way"possible SN",[6] could also be classical nova or something else[9]
SN 1006Lupus17 April 1006 - 1 May 1006–7.5[10]7,200IaMilky WayWidely observed on Earth; in apparent magnitude, the brightest stellar event in recorded history.[11]
SN 1054Taurusc. 10 July [O.S.c. 4 July] 1054
c. 12 April [O.S.c. 6 April] 1056		–6[12]6,500IIMilky WayRemnant is theCrab Nebula with its pulsar (neutron star)
SN 1181Cassiopeia4 August 1181 - 6 August 118107,100sub-luminous Type Iax supernovaMilky WayRemnant is Pa 31 with its hot stellar remnant[13]
SN 1572CassiopeiaNovember 1572–4.08,000IaMilky WayTycho's Nova
SN 1604Ophiuchus8–9 October 1604–314,000IaMilky WayKepler's Supernova; most recent readily visible supernova within the Milky Way
Cas A,
c. 1680		Cassiopeia1680+59,000IIbMilky WayApparently never visually conspicuos, due to interstellar dust; but the remnant,Cas A, is the brightest extrasolar radio source in the sky
G1.9+0.3,
cal. 1868		Sagittarius1868(visible light masked by dust)25,000IaMilky WayLocated near theGalactic Center; "Posthumously" discovered in 1985; age determined in 2008
SN 1885AAndromeda20 August 1885+5.85[14]2,500,000IpecAndromeda GalaxyFirst observation of an extragalactic supernova
SN 1895BCentaurus12 December 1895+8.0[15]10,900,000IaNGC 5253 
SN 1909AUrsa MajorJanuary 1909+12.121,000,000Pinwheel Galaxy (M101)[16][17]
SN 1937CCanes Venatici24 August 1937+8.4[15]13,000,000IaIC 4182 
SN 1939CCepheus17 July 1939+13.025,200,000INGC 6946 (Fireworks Galaxy) 
SN 1940BComa Berenices5 May 1940+12.838,000,000II-PNGC 4725 
SN 1951HUrsa Major1 September 1951+17.521,000,000Pinwheel Galaxy (M101)[18]
SN 1961VPerseus11 July 1961+12.530,000,000II?NGC 1058Potentialsupernova impostor[19]
SN 1970GUrsa Major30 July 1970+12.121,000,000IIPinwheel Galaxy (M101)[20][21][22]
SN 1972ECentaurus13 May 1972+8.7[23]10,900,000IaNGC 5253Followed for more than a year; became the prototypicalType Ia supernova
SN 1983NHydra3 July 1983+11.815,000,000IbMessier 83First observation of aType Ib supernova
SN 1986JAndromeda21 August 1986+18.430,000,000IInNGC 891Bright in the radio frequency range
SN 1987ADorado1987+2.9160,000IIpecLarge Magellanic CloudIntense radiation reached Earth on February 23, 1987, 7:35:35UT. Notable for archival photos of progenitor star and detection ofsupernova neutrinos. Most recentLocal Group supernova
SN 1993JUrsa Major28 March 1993+10.7[24]11,000,000IIbM81One of the brightest supernovae in the northern sky since 1954
SN 1994DVirgo7 March 1994+15.250,000,000IaNGC 4526
SN 1998bwTelescopium26 April 1998?140,000,000IcESO 184-G82Linked toGRB 980425, which was the first time a gamma-ray burst has been linked to a supernova.
SN 1999ehLynx12 October 1999+18.3 +/- 0.384,000,000 INGC 2770First supernovae in this galaxy, where 3 more were detected later.
SN 2002bjLupus2002+14.7160,000,000IInNGC 1821AM Canum Venaticorum-type outburst.[25]
SN 2002ddUrsa Major2002+24.08,000,000,000Iaanonymous galaxyFurthest supernova observed throughHubble Deep Field.[26]
SN 2003fgBoötes20034,000,000,000Iaanonymous galaxyAlso known as the "Champagne supernova"
SN 2004amUrsa MajorMarch 200411,500,000IIM82 (Cigar Galaxy)[27]
SN 2004djCamelopardalis31 July 2004
18:15		8,000,000II-PNGC 2403NGC 2403 is an outlying member of the M81 Group
SN 2213-1745AquariusNovember 2004-June 2005II[28]
SN 2005apComa Berenices3 March 20054,700,000,000II?Announced in 2007 to be the brightest supernova up to that point.
SN 2005gjCetus27 September 2005865,000,000Ia/II-n?Notable for having characteristics of both Type Ia and Type IIn.
SN 2005glPisces5 October 2005+16.5200,000,000II-nNGC 266Star could be found on old pictures.[29]
SN 2006gyPerseus18 September 2006+15240,000,000IIn (*)NGC 1260Observed by NASA,
*with a peak of over 70 days, possibly a new type.
SN 2006jcLynx9 October 200677,000,000IbnUGC 4904
SN 2007biVirgoEarly 2007+18.3Iaanonymous dwarf galaxyExtremely bright and long-lasting, the first good observational match for thepair-instability supernova model postulated for stars of initial mass greater than 140 solar masses (even better than SN 2006gy). The precursor is estimated at 200 solar masses, similar to the first stars of the early universe.[30]
SN 2007uyLynx31 December 2007+16.884,000,000IbcNGC 2770Got overshadowed by SN 2008D.
SN 2008DLynx9 January 200888,000,000IbcNGC 2770First supernova to be observed while it exploded.
MENeaC Abell399.3.14.0Aries+28.71,000,000,000
(z=0.0613)		Iaanonymous red globular cluster associated with anonymous red elliptical galaxy in clusterAbell 399Observed in 2009. Supernova associated with aglobular cluster[31][32]
SN 2009ipPiscis Austrinus200966,000,000IInNGC 7259In 2009 classified as supernova. Redesignated asLuminous blue variable (LBV)Supernova impostor.[33] In September 2012 classified as a young type IIn supernova.[34]
SN 2010ltCamelopardalis2 January 2011+17.0240,000,000Ia (sub-luminous)UGC 3378Discovered by10-year-old girl, the youngest person to discover a supernova.
SN 2011feUrsa Major24 August 2011+10.021,000,000IaM101One of the very few extragalactic supernovae visible in 50mm binoculars.
SN UDS10WilCetusApril 201316,600,000,000Also Known as SN Wilson.[35]

[36][37][38]

SN 2014JUrsa MajorMid January 2014+10.111,500,000IaM82Closest supernova sinceSN 2004dj inNGC 2403.
SN 2014aaLeo7 March 2014310,000,000IaNGC 3861[39][40][41]
SN RefsdalLeo11 November 201414,400,000,000SP 1149It is the first detectedmultiply-lensedsupernova, visible within the field of thegalaxy clusterMACS J1149+2223.[42][43][44][45]
ASASSN-15gaVirgo1 April 20151,000,000,000IaNGC 4866[46]
ASASSN-15lh SN 2015LIndus14 June 2015+16.93,800,000,000IcAPMUKS(BJ) B215839.70−615403.9Most luminoushypernova ever observed.
IPTF14hlsUrsa MajorSeptember 2014+17.7509,000,000unknownSDSS J092034.44+504148.7 (possible dwarf galaxy)Unusual supernova
SN 2016apsDraco22 February 2016+18.113,600,000,000SLSB-II?Most luminous supernova-like event to date.
SN 2017gaxDorado14 August 2017517,000,000 INGC 1672
SN 2018gvPuppis15 January 201870,000,000IaNGC 2525[47][48][49][50][51]
SN 2018zdCamelopardalis2 March 2018+17.870,000,000Ia-csmNGC 2146Firstelectron capture supernova ever detected
SN 2018cowHercules16 June 2018, 10:35:02200,000,000IbCGCG 137-068[52]
SN 2019npLeo Minor9 January 2019+13.075,000,000 IaNGC 3254[53][54]
SN 2019hgpBoötes+20.16920,000,000IcnFirst detected supernova of aWolf-Rayet star[55][56]
SN 2020oiComa Berenices7 January 2020+17.2846,000,000IcMessier 100[citation needed]
SN 2020fqvVirgo31 March 2020+19.059,400,000IIbNGC 4568Earliest known observation of an explosion, 26 hours after[57][58][59]
SN 2020jfoVirgo6 May 202045,610,000IIM61[60][61][62]
SN 2020tlfBoötes2020+15.89120,000,000IInNGC 5731First red supergiant observed before, during and after explosion; earliest known observation, at 130 days before explosion[63][64]
SN 2021gmjUrsa Major20 March 2021+11.234,800,000II-PNGC 3310[65]
SN 2021hprDracoApril 2, 2021129,000,000 ± 29IaNGC 3147[66]
SN 2021jadLepusApril 202165,000,000IaNGC 1964[67]
SN 2021yjaEridanus8 September 2021750,000,000IINGC 1325[68][69]
SN 2021aefxDorado11 November 2021+17.269,000,000IaNGC 1566[70]
SN 2021afdxSculptor23 November 2021+18.8500,000,000IICartwheel Galaxy[71][72]
SN 2022jliCetus5 May 2022+1475,000,000type I-cNGC 157Type Ic, shows periodicity[73][74][75][76]
SN 2022aajnGeminiNovember 2022600,000,000Ia[77]
SN 2023ixfUrsa Major19 May 2023
17:27		+10.821,000,000type II-LPinwheel Galaxy (M101)[78]Closest and brightest supernova sinceSN 2014J
SN 2023rveFornax8 September 2023+13.9450,000,000IINGC 1097[79][80][81][82][83]Brightest Supernova SinceSN 2023ixf.
SN 2023vylPegasus28 October 2023783,000,000IaNGC 7625[84][85]
SN 2023abdgGrus12 December 2023816,000,000IINGC 7421[86]
SN 2023ufx+15.55 IIThe mostmetal-poor supernova found to date.[87]
SN H0peUrsa Major2023IaPLCK G165.7+67.0 Arc 1[88]
SN 2024gyVirgo4 January 2024+12.855,000,000 IaNGC 4216[89]
SN 2024ggiHydra11 April 2024+11.921,700,000 IINGC 3621[90]
SN 2024invLeo10 May 2024+12.182,200,000 IaNGC 3524[91]
SN 2024muvVirgo26 June 2024+12.765,000,000 IaNGC 4699[92]
SN 2024abflCamelopardalis15 November 202441,000,000 IINGC 2146[93]
SN 2025fvwSerpens26 March 2025+13.8100,000,000 IaNGC 5957[94]

Supernova statistics

[edit]
Yearly extragalactic supernovae reported
YearTotalType IType IILBV
(imposters)		Brighter than
apmag 13		Apmag of brightest
Supernova of that year
2024[95]2376616754734511.9 (2024ggi inNGC 3621)
2023[96]1985914304177210.9 (2023ixf inMessier 101)
2022[97]2136817323967412.3 (2022hrs inNGC 4647)
2021[98]2366518494655812.0 (2021aefx inNGC 1566)
2020[99]2177516484517711.8 (2020ue inNGC 4636)
2019[100]1876716524859113.0 (2019np inNGC 3254)
2018[101]952512063327512.7 (2018pv inNGC 3941)
2017[102]82937462184311.5 (2017cbv inNGC 5643)
2016[103]77376812263013.0 (2016coj inNGC 4125)
2015[104]44747072144212.9 (2015F inNGC 2442)
2014[105]22435281752310.1 (2014J inMessier 82)
2013[106]19224981907611.3 (2013aa inNGC 5643)
2012[107]12235501528511.9 (2012fr inNGC 1365)
2011[108]11294391601079.9 (2011fe inMessier 101)
2010[109]9312791357212.8 (2010ih in NGC 2325)
2009[110]5762021371013.0 (2009ig inNGC 1015)
2008[111]5112511431312.4 (2008ge in NGC 1527)
2007[112]6054421301312.0 (2007it in NGC 5530)
2006[113]5584181242312.1 (2006dd inNGC 1316)
2005[114]385273941212.3 (2005df inNGC 1559)
2004[115]343221790211.2 (2004dj inNGC 2403)
2003[116]384198891112.3 (2003hv in NGC 1201)
2002[117]353163640112.3 (2002ap inMessier 74)
2001[118]310108750212.3 (2001e1 inNGC 1448)
2000[119]19976491013.1 (2000cx inNGC 528)
2000–2023147,13516,297
(76.5%)		50009572

See also

[edit]

References

[edit]
  1. ^Modern estimates vary widely; seeSN 185 for more detail.
  2. ^Ksenofontov, L. T.; Berezhko, E. G.; Völk, H. J. (2005-04-01). "Magnetic field amplification in Tycho and other shell-type supernova remnants".Astronomy & Astrophysics.433 (1):229–240.arXiv:astro-ph/0409453.Bibcode:2005A&A...433..229V.doi:10.1051/0004-6361:20042015.ISSN 0004-6361.S2CID 16726273.
  3. ^"New evidence links stellar remains to oldest recorded supernova" Chandra X-ray Observatory, released 2006-09-18, revised 2009-02-20, retrieved 2010-02-26.
  4. ^Chin YN, Huang YL (1994)."Identification of the Guest Star of AD 185 as a comet rather than a supernova".Nature.371 (6496):398–399.Bibcode:1994Natur.371..398C.doi:10.1038/371398a0.S2CID 4240119. Archived fromthe original on 2013-11-05.
  5. ^Zhao FY, Strom RG, Jiang SY (2006)."The Guest Star of AD185 Must Have Been a Supernova".Chinese Journal of Astronomy and Astrophysics.6 (5):635–40.Bibcode:2006ChJAA...6..635Z.doi:10.1088/1009-9271/6/5/17.
  6. ^ab"SNR Cat - U Manitoba".
  7. ^SEDS."Supernova 386".
  8. ^National Radio Astronomy Observatory (NRAO)."The Supernova of 386 AD". Archived fromthe original on 2018-10-06. Retrieved2012-09-02.
  9. ^abHoffmann, Susanne M; Vogt, Nikolaus (2020-09-11)."A search for the modern counterparts of the Far Eastern guest stars 369 CE, 386 CE and 393 CE".Monthly Notices of the Royal Astronomical Society.497 (2):1419–1433.arXiv:2007.01013.Bibcode:2020MNRAS.497.1419H.doi:10.1093/mnras/staa1970.ISSN 0035-8711.
  10. ^Winkler, P. Frank; Gupta, Gaurav; Long, Knox S. (2003). "The SN 1006 Remnant: Optical Proper Motions, Deep Imaging, Distance, and Brightness at Maximum".The Astrophysical Journal.585 (1):324–335.arXiv:astro-ph/0208415.Bibcode:2003ApJ...585..324W.doi:10.1086/345985.S2CID 1626564.
  11. ^"Astronomers Peg Brightness of History's Brightest Star" (Press release). National Optical Astronomy Observatory. 2003-03-05. Archived fromthe original on 2003-04-02. Retrieved2009-01-12.
  12. ^SEDS,Supernova 1055 – Creation of the Crab Nebula
  13. ^Ritter, Andreas; Parker, Quentin A.; Lykou, Foteini; Zijlstra, Albert A.; Guerrero, Martín A.; Le Dû, Pascal (2021-09-01)."The Remnant and Origin of the Historical Supernova 1181 AD".The Astrophysical Journal Letters.918 (2): L33.arXiv:2105.12384.Bibcode:2021ApJ...918L..33R.doi:10.3847/2041-8213/ac2253.hdl:10261/255617.ISSN 2041-8205.S2CID 235195784.
  14. ^de Vaucouleurs, G.; Corwin Jr., H. G. (1985)."S Andromedae 1885 - A centennial review".Astrophysical Journal.295: 287.Bibcode:1985ApJ...295..287D.doi:10.1086/163374.
  15. ^ab"List of Supernovae".Central Bureau for Astronomical Telegrams.Harvard University. Retrieved2021-07-09.
  16. ^Wolf, M. (1909). "Var. 6.1909 Ursae majoris".Astronomische Nachrichten.180 (14–15): 245.Bibcode:1909AN....180..245W.doi:10.1002/asna.19091801405.
  17. ^"SN 1909A".Transient Name Server.IAU. Retrieved25 November 2024.
  18. ^Bishop, David."Other Supernovae images, entry for SN 1951H".Rochester Astronomy. Retrieved25 November 2024.
  19. ^Voisey, Jon (5 November 2010)."What was SN 1961V?".Universe Today. Retrieved1 August 2011.
  20. ^Stoyan, Ronald Atlas of the Messier Objects, Cambridge University Press 2008 page 329
  21. ^Detre, L; Lovas, Miklos (1970)."IAUC 2269".International Astronomical Union Circular (2269): 1.
  22. ^Stienon, Francis; Wdowiak, Thomas (1971). "The Spectrum of the July 1970 Supernova in M101".Information Bulletin on Variable Stars.505: 1.Bibcode:1971IBVS..505....1S.
  23. ^Ardeberg, A.; de Groot, M. (1973). "The 1972 supernova in NGC 5253. Photometric results from the first observing season".Astronomy & Astrophysics.28:295–304.Bibcode:1973A&A....28..295A.
  24. ^J. C. Wheeler; E. Barker; R. Benjamin; J. Boisseau; A. Clocchiatti; G. de Vaucouleurs; N. Gaffney; R. P. Harkness; A. M. Khokhlov; D. F. Lester; B. J. Smith; V. V. Smith; J. Tomkin (1993). "Early Observations of SN 1993J in M81 at McDonald Observatory".Astrophysical Journal.417:L71 –L74.Bibcode:1993ApJ...417L..71W.doi:10.1086/187097.
  25. ^Sanders, Robert."Rapid supernova could be new class of exploding star".UC Newsroom. University of California, Berkeley. Archived fromthe original on 2011-06-13. Retrieved2009-11-06.
  26. ^information@eso.org."SN2002dd in the HDF North - 2002".www.esahubble.org. Retrieved2024-08-17.
  27. ^"SN 2004am | Transient Name Server".wis-tns.weizmann.ac.il. Retrieved14 July 2020.
  28. ^Cooke, J.; Sullivan, M.; Gal-Yam, A.; Barton, E. J.; Carlberg, R. G.;Ryan-Weber, E. V.; Horst, C.; Omori, Y.; Díaz, C. G. (2012). "Superluminous supernovae at redshifts of 2.05 and 3.90".Nature.491 (7423):228–231.arXiv:1211.2003.Bibcode:2012Natur.491..228C.doi:10.1038/nature11521.PMID 23123848.S2CID 4397580.
  29. ^David Bishop (2005)."Supernova 2005gl in NGC 266".Central Bureau Electronic Telegrams (250). Rochester Academy of Science: 1.Bibcode:2005CBET..250....1P. Retrieved26 August 2012.
  30. ^Science Daily,"Superbright Supernova Is First of Its Kind", 5 December 2009 (accessed 2009-12-15)
  31. ^Melissa L. Graham; David J. Sand; Dennis Zaritsky; Chris J. Pritchet (13 May 2015). "Confirmation of Hostless Type Ia Supernovae Using Hubble Space Telescope Imaging".The Astrophysical Journal.807 (1): 83.arXiv:1505.03407.Bibcode:2015ApJ...807...83G.doi:10.1088/0004-637X/807/1/83.S2CID 118555601.
  32. ^Robert Sanders (4 June 2015)."Exiled stars explode far from home". UC Berkeley News Center. Archived fromthe original on 12 June 2015. Retrieved6 June 2015.
  33. ^"Supernova impostor explodes for real".www.newscientist.com. RetrievedNovember 29, 2017.
  34. ^Maza, J.; Hamuy, M.; Antezana, R.; Gonzalez, L.; Lopez, P.; Silva, S.; Folatelli, G.; Iturra, D.; Cartier, R.; Forster, F.; Marchi, S.; Rojas, A.; Pignata, G.; Conuel, B.; Reichart, D.; Ivarsen, K.; Haislip, J.; Crain, A.; Foster, D.; Nysewander, M.; Lacluyze, A. (2009)."Supernova 2009ip in NGC 7259".Central Bureau Electronic Telegrams (1928): 1.Bibcode:2009CBET.1928....1M. Archived fromthe original on September 11, 2016. RetrievedNovember 29, 2017.
  35. ^Major, Jason (5 April 2013)."Hubble Spots the Most Distant Supernova Ever".Discovery Channel. Archived fromthe original on 26 March 2016. Retrieved28 June 2015.
  36. ^Yglesias, Matthew (2013-04-04)."Exploding stars: Supernova found is most distant of its kind yet". Slate.com. Retrieved2013-04-08.
  37. ^"Hubble breaks record for furthest supernova".esahubble.org. 2013-04-04. Retrieved2024-08-31.
  38. ^Jones, David O.; Rodney, Steven A.; Riess, Adam G.; Mobasher, Bahram; Dahlen, Tomas; McCully, Curtis; Frederiksen, Teddy F.; Casertano, Stefano; Hjorth, Jens; Keeton, Charles R.; Koekemoer, Anton; Strolger, Louis-Gregory; Wiklind, Tommy G.; Challis, Peter; Graur, Or (25 April 2013)."The Discovery of the Most Distant Known Type Ia Supernova at Redshift 1.914".The Astrophysical Journal.768 (2): 166.arXiv:1304.0768.Bibcode:2013ApJ...768..166J.doi:10.1088/0004-637X/768/2/166.ISSN 0004-637X.
  39. ^"Bright Supernovae - 2014".rochesterastronomy.org. Retrieved2018-07-28.
  40. ^"SN 2014aa | Transient Name Server".wis-tns.weizmann.ac.il. Retrieved2018-07-28.
  41. ^"2014aa - The Open Supernova Catalog".sne.space. Archived fromthe original on 2018-07-28. Retrieved2018-07-28.
  42. ^Kelly, P. L.; Rodney, S. A.; Treu, T.; Foley, R. J.; Brammer, G.; Schmidt, K. B.; Zitrin, A.; Sonnenfeld, A.; Strolger, L. -G.; Graur, O.; Filippenko, A. V.; Jha, S. W.; Riess, A. G.; Bradac, M.; Weiner, B. J.; Scolnic, D.; Malkan, M. A.; von Der Linden, A.; Trenti, M.; Hjorth, J.; Gavazzi, R.; Fontana, A.; Merten, J. C.; McCully, C.; Jones, T.; Postman, M.; Dressler, A.; Patel, B.; Cenko, S. B.; et al. (2015). "Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens".Science.347 (6226):1123–1126.arXiv:1411.6009.Bibcode:2015Sci...347.1123K.doi:10.1126/science.aaa3350.PMID 25745167.S2CID 206633888.
  43. ^Overbye, Dennis (March 5, 2015)."Astronomers Observe Supernova and Find They're Watching Reruns".New York Times. RetrievedMarch 5, 2015.
  44. ^Amina Khan (5 March 2015)."Don't believe the light: Supernova in 'Einstein Cross' is a cosmic trick".Los Angeles Times.
  45. ^Sharon, K.; Johnson, T. L. (2015). "Revised Lens Model for the Multiply Imaged Lensed Supernova, "Sn Refsdal" in Macs J1149+2223".The Astrophysical Journal.800 (2): L26.arXiv:1411.6933.Bibcode:2015ApJ...800L..26S.doi:10.1088/2041-8205/800/2/L26.S2CID 118735742.
  46. ^Piascik, A. S.; Steele, I. A. (2015-01-01)."ATel #7333: Spectral Classification of ASASSN-15ga in NGC4866".The Astronomer's Telegram. Retrieved2021-02-02.
  47. ^"SN 2018gv".Transient Name Server.IAU. Retrieved9 December 2024.
  48. ^Siebert, M. R.; Dimitriadis, G.; Foley, R. J. (2018)."Spectroscopic Classification of SN 2018gv with Keck I/LRIS".The Astronomer's Telegram.11175: 1.Bibcode:2018ATel11175....1S.
  49. ^Bufano, F.; Berton, M.; Vogl, C.; Floers, A.; Taubenberger, S.; Anderson, J.; Galbany, L.; Schulze, S.; Yaron, O.; Manulis, I.; Inserra, C.; Kankare, E.; Maguire, K.; Smartt, S. J.; Young, D.; Smith, K. W.; McBrien, O.; Tonry, J.; Denneau, L.; Heinze, A.; Weiland, H.; Stalder, B.; Rest, A. (2018)."EPESSTO spectroscopic classification of optical transients: SN2018gv a very young SN Ia".The Astronomer's Telegram.11177: 1.Bibcode:2018ATel11177....1B.
  50. ^"Time-Lapse of Supernova in NGC 2525",European Space Agency, retrieved2021-11-05
  51. ^NASA, ESA, J. DePasquale (STScI), M. Kornmesser and M. Zamani (ESA/Hubble), A. Riess (STScI/JHU) and the SH0ES team, and the Digitized Sky Survey (6 October 2020)."Check out this exploding supernova captured by the Hubble telescope".CBBC Newsround.Supernova SN 2018gv{{cite web}}: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link)
  52. ^Morris, Amanda (26 May 2020)."Astrophysicists capture new class of transient objects".Phys.org. Retrieved26 May 2020.
  53. ^"SN 2019np".Transient Name Server.IAU. Retrieved27 November 2024.
  54. ^Bishop, David."Bright Supernovae - 2019".Rochester Astronomy. Retrieved9 December 2024.
  55. ^Gal-Yam, A.; Bruch, R.; Schulze, S.; Yang, Y.; Perley, D. A.; Irani, I.; Sollerman, J.; Kool, E. C.; Soumagnac, M. T.; Yaron, O.; Strotjohann, N. L. (12 January 2022)."A WC/WO star exploding within an expanding carbon–oxygen–neon nebula".Nature.601 (7892):201–204.arXiv:2111.12435.Bibcode:2022Natur.601..201G.doi:10.1038/s41586-021-04155-1.ISSN 1476-4687.PMID 35022591.S2CID 244527654.
  56. ^"Astronomers discover first supernova explosion of a Wolf-Rayet star".Instituto de Astrofísica de Canarias • IAC. 12 January 2022. Retrieved2022-02-08.
  57. ^Jenner, Lynn (2021-10-19)."Hubble Gives Unprecedented, Early View of a Doomed Star's Destruction".NASA. Retrieved2021-11-05.
  58. ^Gough, Evan (2021-10-29)."Quick Action Let Hubble Watch the Earliest Stages of an Unfolding Supernova Detonation".Universe Today. Retrieved2021-11-05.
  59. ^Tinyanont, Samaporn; Ridden-Harper, R; Foley, R J; Morozova, V; Kilpatrick, C D; Dimitriadis, G; DeMarchi, L; Gagliano, A; Jacobson-Galán, W V; Messick, A; Pierel, J D R (2021-10-26)."Progenitor and close-in Circumstellar Medium of Type II Supernova 2020fqv from high-cadence photometry and ultra-rapid UV spectroscopy".Monthly Notices of the Royal Astronomical Society.512 (stab2887):2777–2797.arXiv:2110.10742.doi:10.1093/mnras/stab2887.ISSN 0035-8711.
  60. ^Sollerman, J. (2021-07-30). "The Type II supernova SN 2020jfo in M 61, implications for progenitor system, and explosion dynamics".Astronomy & Astrophysics.655: A105.arXiv:2107.14503.Bibcode:2021A&A...655A.105S.doi:10.1051/0004-6361/202141374.S2CID 239388865.
  61. ^Vallely, P.J.; Kocanek, CS; Stanek, KZ; Fausnaugh, M; Shappee, BJ (February 2021)."High-cadence, early-time observations of core-collapse supernovae from the TESS prime mission".Monthly Notices of the Royal Astronomical Society.500 (4):5639–5656.arXiv:2010.06596.doi:10.1093/mnras/staa3675.
  62. ^Jones, DO (2021)."The Young Supernova Experiment: Survey Goals, Overview, and Operations".The Astrophysical Journal.908 (143): 143.arXiv:2010.09724.Bibcode:2021ApJ...908..143J.doi:10.3847/1538-4357/abd7f5.S2CID 224803297.
  63. ^Jacobson-Galán, W. V.; Dessart, L.; Jones, D. O.; Margutti, R.; Coppejans, D.L.; Dimitriadis, G.; Foley, R. J.; Kilpatrick, C. D.; Matthews, D. J.; Rest, S.; Terreran, G.; Aleo, P. D.; Auchettl, K.; Blanchard, P. K.; Coulter, D. A.; Davis, K. W.; de Boer, T. J. L.; DeMarchi, L.; Drout, M. R.; Earl, N.; Gagliano, A.; Gall, C.; Hjorth, J.; Huber, M. E.; Ibik, A. L.; Milisavljevic, D.; Pan, Y.-C.; Rest, A.; Ridden-Harper, R.; Rojas-Bravo, C.; Siebert, M. R.; Smith, K. W.; Taggart, K.; Tinyanont, S.; Wang, Q.; Zenati, Y. (6 January 2022)."Final Moments. I. Precursor Emission, Envelope Inflation, and Enhanced Mass Loss Preceding the Luminous Type II Supernova 2020tlf".The Astrophysical Journal.924 (1). American Astronomical Society: 15.arXiv:2109.12136.Bibcode:2022ApJ...924...15J.doi:10.3847/1538-4357/ac3f3a.S2CID 237940678.
  64. ^Anderson, Paul Scott (14 January 2022)."Dying star's explosive end seen by astronomers".EarthSky. Deborah Byrd. Retrieved16 January 2022.
  65. ^"SN 2021gmj".Transient Name Server. Retrieved2021-12-20.
  66. ^Bishop, David (May 13, 2021)."Supernovae 2021jad in NGC 1964".Rochester Astronomy. Rochester Academy of Science. Retrieved2021-12-19.
  67. ^Bishop, David (May 13, 2021)."Supernovae 2021jad in NGC 1964".Rochester Astronomy. Rochester Academy of Science. Retrieved2021-12-19.
  68. ^Smith, K. W.; et al. (September 2021). "ATLAS21bidw (AT2021yja): discovery of a candidate SN in NGC 1325 (22 Mpc)".Transient Name Server AstroNote 2021-235.235: 1.Bibcode:2021TNSAN.235....1S.
  69. ^Ryder, S. D.; et al. (September 2021). "Radio observations of SN 2021yja".The Astronomer's Telegram.14915: 1.Bibcode:2021ATel14915....1R.
  70. ^"Bright Supernovae - 2021".www.rochesterastronomy.org. Retrieved21 January 2024.
  71. ^David Bishop (23 November 2021)."2021afdx".rochesterastronomy.org. Retrieved28 November 2021.
  72. ^"SN 2021afdx".Transient Name Server. IAU Supernova Working Group. 23 November 2021. Retrieved28 November 2021.
  73. ^Moore, T.; et al. (October 2023)."SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise".The Astrophysical Journal Letters.956 (1): L31.arXiv:2309.12750.Bibcode:2023ApJ...956L..31M.doi:10.3847/2041-8213/acfc25.ISSN 2041-8205.
  74. ^Chen, Ping; et al. (January 2024)."A 12.4-day periodicity in a close binary system after a supernova".Nature.625 (7994):253–258.arXiv:2310.07784.Bibcode:2024Natur.625..253C.doi:10.1038/s41586-023-06787-x.ISSN 1476-4687.PMID 38200292.S2CID 263909264. Retrieved12 January 2024.
  75. ^"Missing link found: supernovae give rise to black holes or neutron stars".www.eso.org. Retrieved12 January 2024.
  76. ^"Supernova 2022jli in NGC 157".www.rochesterastronomy.org. Retrieved12 January 2024.
  77. ^"SN 2022aajn".ESA. Retrieved18 October 2024.
  78. ^O'Callaghan, Jonathan (October 2023). "Out with a Bang".Scientific American.329 (3):8–11.doi:10.1038/scientificamerican1023-8.PMID 39017247.
  79. ^Odeh, Mohammad (8 September 2023)."AT 2023rve".IAU Supernova Working Group. Retrieved10 September 2023.
  80. ^Arrizabalaga, P. (12 September 2023)."SN 2023rve: follow-up photometry with LCOGT DeltaRho 350 + QHY600".IAU Supernova Working Group. Retrieved14 September 2023.
  81. ^Bishop, David (12 September 2023)."Supernovae 2023rve in NGC 1097".Bright Supernovae. Retrieved14 September 2023.
  82. ^Otero, Sebastian (12 September 2023)."The International Variable Star Index: SN 2023rve".AAVSO. Retrieved14 September 2023.
  83. ^Ghannam, Osama (8 September 2023)."New Supernova is Discovered From the UAE".IAC. Retrieved14 September 2023.
  84. ^Supernovae 2023vyl in NGC 7625, Astronomy Section, Rochester Academy of Science, January 26, 2024, retrieved2024-01-28.
  85. ^"SN 2023vyl".Transient Name Server.IAU. Retrieved14 August 2024.
  86. ^"SN 2023abdg",Transient Name Server, retrieved2024-02-04.
  87. ^Tucker, Michael A.; Hinkle, Jason; Angus, Charlotte R.; Auchettl, Katie; Hoogendam, Willem B.; Shappee, Benjamin; Kochanek, Christopher S.; Ashall, Chris; Boer, Thomas de; Chambers, Kenneth C.; Desai, Dhvanil D.; Do, Aaron; Fulton, Michael D.; Gao, Hua; Herman, Joanna (2024)."The Extremely Metal-poor SN 2023ufx: A Local Analog to High-redshift Type II Supernovae".The Astrophysical Journal.976 (2): 178.arXiv:2405.00113.Bibcode:2024ApJ...976..178T.doi:10.3847/1538-4357/ad8448.ISSN 0004-637X.
  88. ^Polletta, M.; Nonino, M.; Frye, B.; et al. (July 2023). "Spectroscopy of the supernova H0pe host galaxy at redshift 1.78".Astronomy & Astrophysics.675: L4.arXiv:2306.12385.Bibcode:2023A&A...675L...4P.doi:10.1051/0004-6361/202346964.S2CID 259212330.
  89. ^"SN 2024gy".Transient Name Server.IAU. Retrieved17 December 2024.
  90. ^"SN 2024ggi".Transient Name Server.IAU. Retrieved4 December 2024.
  91. ^"SN 2024inv".Transient Name Server.IAU. Retrieved16 December 2024.
  92. ^"SN 2024muv".Transient Name Server.IAU. Retrieved27 November 2024.
  93. ^"SN 2024abfl".Transient Name Server.IAU. Retrieved15 November 2024.
  94. ^"2025fvw | Transient Name Server".www.wis-tns.org. Retrieved31 March 2025.
  95. ^David Bishop."Supernova discovery statistics for 2024". Retrieved2024-03-24.
  96. ^David Bishop."Supernova discovery statistics for 2023". Retrieved2023-01-11.
  97. ^David Bishop."Supernova discovery statistics for 2022". Retrieved2023-02-18.
  98. ^David Bishop."Supernova discovery statistics for 2021". Retrieved2023-02-18.
  99. ^David Bishop."Supernova discovery statistics for 2020". Retrieved2023-02-18.
  100. ^David Bishop."Supernova discovery statistics for 2019". Retrieved2023-02-18.
  101. ^David Bishop."Supernova discovery statistics for 2018". Retrieved2023-02-18.
  102. ^David Bishop."Supernova discovery statistics for 2017". Retrieved2023-02-20.
  103. ^David Bishop."Supernova discovery statistics for 2016". Retrieved2023-02-20.
  104. ^David Bishop."Supernova discovery statistics for 2015". Retrieved2023-02-20.
  105. ^David Bishop."Supernova discovery statistics for 2014". Retrieved2023-02-20.
  106. ^David Bishop."Supernova discovery statistics for 2013". Retrieved2023-02-20.
  107. ^David Bishop."Supernova discovery statistics for 2012". Retrieved2023-02-21.
  108. ^David Bishop."Supernova discovery statistics for 2011". Retrieved2023-02-21.
  109. ^David Bishop."Supernova discovery statistics for 2010". Retrieved2023-02-21.
  110. ^David Bishop."Supernova discovery statistics for 2009". Retrieved2023-02-21.
  111. ^David Bishop."Supernova discovery statistics for 2008". Retrieved2023-02-21.
  112. ^David Bishop."Supernova discovery statistics for 2007". Retrieved2023-02-21.
  113. ^David Bishop."Supernova discovery statistics for 2006". Retrieved2023-02-21.
  114. ^David Bishop."Supernova discovery statistics for 2005". Retrieved2023-02-23.
  115. ^David Bishop."Supernova discovery statistics for 2004". Retrieved2023-02-23.
  116. ^David Bishop."Supernova discovery statistics for 2003". Retrieved2023-02-23.
  117. ^David Bishop."Supernova discovery statistics for 2002". Retrieved2023-02-23.
  118. ^David Bishop."Supernova discovery statistics for 2001". Retrieved2023-02-23.
  119. ^David Bishop."Supernova discovery statistics for 2000". Retrieved2023-02-23.

Further reading

[edit]
  • Green, David A. (2015). Orchiston, Wayne; Green, David A.; Strom, Richard (eds.).Historical Supernova Explosions in Our Galaxy and Their Remnants.New Insights From Recent Studies in Historical Astronomy: Following in the Footsteps of F. Richard Stephenson, Astrophysics and Space Science Proceedings. Astrophysics and Space Science Proceedings. Vol. 43. Switzerland: Springer International Publishing. pp. 91–100.doi:10.1007/978-3-319-07614-0_7.ISBN 978-3-319-07613-3.

External links

[edit]
Classes
Physics of
Related
Progenitors
Remnants
Discovery
Lists
Notable
Research
Portals:
Retrieved from "https://en.wikipedia.org/w/index.php?title=List_of_supernovae&oldid=1312494466"
Categories:
Hidden categories:
[8]ページ先頭
©2009-2025 Movatter.jp