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  • ...Yu. P. | title = Photometric classification and basic parameters of type I supernovae | journal = [[Astronomy Reports|Soviet Astronomy]] | volume = 28 | pages = ...ne the decline after the maximum light was rather simple for most observed supernovae. ...
    6 KB (845 words) - 22:43, 26 October 2024
  • .... Cosmological parameters]</ref>) and direct late-time measurements from [[supernovae]] (e.g. from Reiss et al. 2022<ref>[https://iopscience.iop.org/article/10.3 ...
    7 KB (927 words) - 14:32, 25 November 2024
  • ...ion is that something else is happening to these extra large stars. Failed supernovae and black hole formation is one proposed explanation.<ref name=adams/> If t ...|last4=Stanek|first4=K. Z.|last5=Dai|first5=X.|title=The search for failed supernovae with the Large Binocular Telescope: confirmation of a disappearing star|jou ...
    7 KB (1,051 words) - 03:45, 24 January 2025
  • ...t curve]] for V1104 Scorpii, plotted from ''[[All Sky Automated Survey for SuperNovae|ASAS-SN]]'' data<ref name="ASAS-SN"/> ...ution of these stars is critical to the interpretation and modeling of the supernovae they produce.<ref name="richardson" /> ...
    7 KB (1,006 words) - 20:58, 24 October 2024
  • ...no]]s (and anti-neutrinos) cumulatively originating from all core-collapse supernovae events throughout the history of the universe. Though it has not yet been d ...s source of neutrinos accumulated from all of the individual core-collapse supernovae throughout the history of the universe. Due to uncertainties in the emitted ...
    15 KB (2,190 words) - 10:52, 8 February 2025
  • ...niv. of Arizona Press |isbn=0-8165-1825-4 |oclc=246985772}}</ref> In these supernovae, these winds are a result of the conversion of the supernova's [[thermal en ...
    5 KB (791 words) - 05:22, 17 November 2024
  • ...ion=Cambridge, United Kingdom|oclc=1153342277}}</ref> Supernovae{{efn|'''''Supernovae''''' is the plural of ''supernova'', used in most academic sources. Less fo ...dromeda Galaxy|Andromeda]] or beyond.<ref name=":14" /> The observation of supernovae will broaden our understanding of various [[Astrophysics|astrophysical]] an ...
    37 KB (5,132 words) - 14:10, 4 October 2024
  • ...t''' ('''LFBOT'''), is an explosive transient event similar to [[Supernova|supernovae]] and [[Gamma-ray burst|gamma-ray bursts]] with high optical luminosity, ra |File:FBOTvsGRBvsSN.jpg|Comparison of explosion scenarios of supernovae (SN), gamma-ray bursts (GRB) and fast blue optical transients (FBOT) ...
    16 KB (2,201 words) - 22:47, 3 September 2024
  • ...eler, J. C. (1997). Deflagration-to-detonation transition in thermonuclear supernovae. The Astrophysical Journal, 478(2), 678.</ref><ref>Oran, E. S., & Gamezo, V ...
    6 KB (984 words) - 00:28, 20 February 2025
  • ...Facility]] (ZTF)<ref name="ZTF" /> and the [[All Sky Automated Survey for SuperNovae]] (ASAS-SN).<ref name=holoien2019>{{cite journal |doi=10.3847/1538-4357/ab3 ...be distinguished from other [[transient astronomical source]]s, such as [[supernovae]]. The peak luminosity of TDEs is proportional to the central black hole ma ...
    21 KB (2,975 words) - 01:39, 7 February 2025
  • ...se in on itself and explode as a [[type Ib and Ic supernovae|type Ib or Ic supernovae]]. Depending on the amount of mass lost before the supernova explosion, th ...
    13 KB (1,939 words) - 23:07, 14 August 2024
  • |title=Measurements of Ω and Λ from 42 High-Redshift Supernovae ...nature of the acceleration, completely independent from the [[Dark energy#Supernovae|supernova technique]]. ...
    26 KB (3,764 words) - 02:43, 21 September 2024
  • ...A. |last2=Uddin |title=Constraining a Possible Variation of G with Type Ia Supernovae |date=10 April 2014 |volume=31 |pages=e015 |doi=10.1017/pasa.2014.9 |journa ...
    18 KB (2,508 words) - 09:37, 23 January 2025
  • ...–86|year=1999|title=Measurements of Omega and Lambda from 42 high redshift supernovae|arxiv=astro-ph/9812133 |doi=10.1086/307221|bibcode=1999ApJ...517..565P|last ...
    15 KB (2,207 words) - 13:17, 2 June 2024
  • ...and star burst strengths. Major syntheses channels of iron are [[Supernova|supernovae]] Ia and II.<ref>{{Cite journal|last1=Burbidge|first1=E. Margaret|last2=Bur ...
    9 KB (1,360 words) - 11:45, 2 September 2024
  • ...] [[light curve]] for HV 2112, plotted from [[All Sky Automated Survey for SuperNovae|ASAS-SN]] data<ref name="ASAS-SN"/>]] ...017PASP..129j4502K|arxiv=1706.07060|title=The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0|journal=Publications of the Astronomical ...
    17 KB (2,439 words) - 19:04, 25 February 2025
  • ...mes the size of our own sun before [[Explosion|exploding]] in catastrophic supernovae. After such an explosion blows a star's outer layers into space, the core r ...
    11 KB (1,746 words) - 18:28, 6 August 2024
  • 10 KB (1,441 words) - 00:47, 12 November 2024
  • ...10.1103/PhysRevLett.83.670| title = Constraining Dark Energy with Type Ia Supernovae and Large-Scale Structure| journal = Physical Review Letters| volume = 83| === Supernovae === ...
    85 KB (11,700 words) - 06:27, 27 February 2025
  • ...ng |first3=Sebastien |title=Dynamics of an Alfven surface in core collapse supernovae |journal=The Astrophysical Journal |date=2010 |volume=729 |issue=1 |page=71 ...
    15 KB (2,118 words) - 17:14, 27 December 2024
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