• Thumbnail for Superluminous supernova
    (CSM model), or pair-instability supernovae. The first confirmed superluminous supernova connected to a gamma ray burst was not found until 2003, when GRB...
    24 KB (2,578 words) - 14:28, 6 September 2024
  • Thumbnail for ASASSN-15lh
    Automated Survey for SuperNovae (ASAS-SN), with the appearance of a superluminous supernova event. It was first detected on June 14, 2015, located within a...
    18 KB (1,939 words) - 04:07, 16 November 2024
  • Thumbnail for Supernova
    of supernova remnants Quark-nova – Hypothetical violent explosion resulting from conversion of a neutron star to a quark star Superluminous supernova –...
    201 KB (21,944 words) - 04:21, 18 November 2024
  • Micronova Supernova Type Ia supernova Type Ib and Ic supernovae Type II supernova Superluminous supernova Pair-instability supernova Hypernova Supernova impostor...
    808 bytes (79 words) - 18:21, 9 February 2024
  • Thumbnail for Gamma-ray burst
    of most observed GRBs is thought to be released during a supernova or superluminous supernova as a high-mass star implodes to form a neutron star or a...
    119 KB (12,993 words) - 23:24, 18 November 2024
  • Thumbnail for Eta Carinae
    radiation, resulting in a superluminous supernova (SLSN) or hypernova, several times more luminous than a typical core collapse supernova and much longer-lasting...
    125 KB (14,963 words) - 20:09, 27 October 2024
  • Thumbnail for SN 2005ap
    supernova in the galaxy SDSS J130115.12+274327.5. With a peak absolute magnitude of around −22.7, it is the second-brightest superluminous supernova yet...
    6 KB (503 words) - 13:01, 15 November 2024
  • Thumbnail for Nova
    Nova (redirect from Nova and Supernova)
    Guest star (astronomy) Hypernova Kilonova Micronova Superluminous supernova Supernova Supernova impostor X-ray burster "Nova Centauri 2013: Another bright...
    28 KB (3,035 words) - 15:20, 25 October 2024
  • "PS1-10afx at z=1.388: Pan-STARRS1 Discovery of a New Type of Superluminous Supernova". The Astrophysical Journal. 767 (2): 162. arXiv:1302.0009. Bibcode:2013ApJ...
    36 KB (3,236 words) - 22:01, 23 July 2024
  • Thumbnail for Pair-instability supernova
    A pair-instability supernova is a type of supernova predicted to occur when pair production, the production of free electrons and positrons in the collision...
    18 KB (2,112 words) - 12:55, 15 November 2024
  • Thumbnail for SN 1000+0216
    SN 1000+0216 was an extremely remote superluminous supernova (SLSN), which occurred in between June and November 2006 in the constellation Sextans. Its...
    3 KB (254 words) - 12:57, 15 November 2024
  • 2017). "The unexpected, long-lasting, UV rebrightening of the superluminous supernova ASASSN-15lh". Monthly Notices of the Royal Astronomical Society...
    140 KB (9,736 words) - 22:00, 31 October 2024
  • Thumbnail for PS1-10adi
    3×1052 ergs (2.3×1045 Joules), exceeding ASASSN-15lh. It may be a superluminous supernova or a stellar disruption event. The magnitude of the explosion challenges...
    5 KB (430 words) - 13:12, 30 July 2023
  • Thumbnail for Indus (constellation)
    Sky Automated Survey for SuperNovae (ASAS-SN) in 2015 detected a superluminous supernova, named ASASSN-15lh (also designated SN 2015L). Based on the study...
    9 KB (848 words) - 21:12, 30 April 2024
  • "pulsational pair instability" supernova or possibly a full pair instability supernova. Superluminous supernova – Supernova at least ten times more luminous...
    6 KB (517 words) - 13:04, 15 November 2024
  • Thumbnail for VY Canis Majoris
    long-lasting type IIn supernova (SN IIn) a hypernova; or a superluminous supernova (SLSN) comparable to SN 1988Z or less likely, a type Ib supernova, but it is unlikely...
    63 KB (6,874 words) - 15:28, 26 October 2024
  • Thumbnail for Jean-Pierre Luminet
    resulting from the accretion of stellar debris. It explains the superluminous supernova SN 2015L, the tidal explosion of a white dwarf before being absorbed...
    19 KB (2,030 words) - 00:43, 5 October 2024
  • Thumbnail for SN 2018cow
    SN 2018cow (redirect from Supernova 2018cow)
    time. Common envelope jets supernova – Supernova caused by a giant and compact star merging Superluminous supernova – Supernova at least ten times more luminous...
    34 KB (3,283 words) - 13:07, 15 November 2024
  • Thumbnail for SN 2006gy
    SN 2006gy was an extremely energetic supernova, also referred to as a hypernova, that was discovered on September 18, 2006. It was first observed by Robert...
    12 KB (1,088 words) - 20:30, 22 August 2024
  • Thumbnail for Blue supergiant
    can execute a number of blue loops before either exploding as a type II supernova or finally dumping enough of its outer layers to become a blue supergiant...
    21 KB (2,513 words) - 04:33, 2 November 2024
  • Thumbnail for Hypernova
    seconds to over a minute in duration. They have also been referred to as superluminous supernovae, though that classification also includes other types of...
    20 KB (2,210 words) - 12:44, 25 August 2024
  • SN 2213-1745 was an extremely remote superluminous supernova (SLSN), which occurred in between November 2004 and June 2005. Its peak far-ultraviolet absolute...
    3 KB (229 words) - 13:07, 15 November 2024
  • Thumbnail for Supernova impostor
    Supernova impostors are stellar explosions that appear at first to be a supernova but do not destroy their progenitor stars. As such, they are a class...
    4 KB (402 words) - 19:03, 10 October 2024
  • Thumbnail for Shrinivas Kulkarni
    succeeded in identifying the new groups of optical transients such as superluminous supernovae, calcium-rich supernovae, and luminous red novae. The success...
    20 KB (1,738 words) - 17:47, 15 August 2024
  • Texas Supernova Search (TSS) is one of many ongoing projects to identify and record supernova events. The project is led by Robert Quimby and to date...
    3 KB (290 words) - 11:11, 17 November 2024
  • Thumbnail for Luminous blue variable
    observed in two or three well-studied stars and possibly a handful of supernova imposters. The two clear examples in the Milky Way galaxy, P Cygni and...
    39 KB (4,826 words) - 10:40, 2 November 2024
  • Thumbnail for Black dwarf
    It is speculated that some massive black dwarfs may eventually produce supernova explosions. These will occur if pycnonuclear (density-based) fusion processes...
    10 KB (1,142 words) - 05:00, 25 July 2024
  • Thumbnail for NGC 2444
    Taggart, K; Perley, D A (5 April 2021). "Core-collapse, superluminous, and gamma-ray burst supernova host galaxy populations at low redshift: the importance...
    5 KB (408 words) - 14:41, 6 September 2024
  • Thumbnail for White dwarf
    been a type Ia supernova from a white dwarf, possibly the merger of two white dwarfs. Tycho's Supernova of 1572 was also a type Ia supernova, and its remnant...
    152 KB (17,712 words) - 12:25, 18 November 2024
  • Thumbnail for Stellar evolution
    Stars with around ten or more times the mass of the Sun can explode in a supernova as their inert iron cores collapse into an extremely dense neutron star...
    50 KB (6,476 words) - 03:27, 27 October 2024