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There is a page named "Core collapse supernova" on Wikipedia

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  • Thumbnail for Supernova
    either collapses to a neutron star or black hole, or is completely destroyed to form a diffuse nebula. The peak optical luminosity of a supernova can be...
    201 KB (21,932 words) - 21:37, 18 August 2024
  • Supernova neutrinos are weakly interactive elementary particles produced during a core-collapse supernova explosion. A massive star collapses at the end...
    37 KB (4,416 words) - 21:51, 19 August 2024
  • Thumbnail for Type II supernova
    A Type II supernova or SNII (plural: supernovae) results from the rapid collapse and violent explosion of a massive star. A star must have at least eight...
    49 KB (4,792 words) - 00:40, 25 August 2024
  • Core collapse can refer to: The collapse of the stellar core of a massive star, such as the core collapse that produces a supernova Core collapse (cluster)...
    304 bytes (76 words) - 19:45, 9 February 2022
  • Thumbnail for Pair-instability supernova
    supporting a supermassive star's core against gravitational collapse. This pressure drop leads to a partial collapse, which in turn causes greatly accelerated...
    18 KB (2,096 words) - 09:21, 15 July 2024
  • is an essential component of supernova nucleosynthesis. A shock wave rebounded from matter collapsing onto the dense core, if strong enough to lead to...
    43 KB (4,797 words) - 16:19, 21 August 2024
  • Thumbnail for UY Scuti
    UY Scuti (section Supernova)
    disrupting the balance of gravity and radiation in its core and resulting in a core collapse supernova. It is expected that a star like UY Scuti should evolve...
    17 KB (1,825 words) - 20:23, 9 August 2024
  • Thumbnail for Kepler's Supernova
    supernova remnant, a type Ia supernova. The abundance of oxygen relative to iron in the remnant of SN 1604 is roughly solar, whereas a core-collapse scenario...
    16 KB (1,675 words) - 11:16, 18 August 2024
  • Thumbnail for Superluminous supernova
    layers of the star, and it will collapse into a black hole without producing a visible supernova outburst. A star with a core mass slightly below this level—in...
    23 KB (2,525 words) - 01:11, 23 August 2024
  • Thumbnail for SN 1987A
    SN 1987A (redirect from Supernova 1987A)
    experiments with artificial neutrino sources. SN 1987A appears to be a core-collapse supernova, which should result in a neutron star given the size of the original...
    47 KB (5,021 words) - 05:53, 28 August 2024
  • Thumbnail for SN 2023ixf
    SN 2023ixf is a type II-L (core collapse) supernova located in the Pinwheel Galaxy. It was first observed on 19 May 2023 by Kōichi Itagaki and immediately...
    8 KB (506 words) - 19:52, 29 July 2024
  • for electron-positron pair creation, where it then undergoes a core-collapse supernova or hypernova. It is possible that this is what occurred during...
    7 KB (1,002 words) - 11:35, 10 September 2023
  • νp-process (nu p process). Massive stars end their life in a core-collapse supernova. In such a supernova, a shockfront from an explosion runs from the center...
    36 KB (3,656 words) - 15:08, 20 August 2024
  • Thumbnail for R-process
    suggested the material ejected from the reexpanded core of a core-collapse supernova, as part of supernova nucleosynthesis, or decompression of neutron star...
    31 KB (3,894 words) - 12:57, 23 August 2024
  • Thumbnail for Hypernova
    energetic supernova which is believed to result from an extreme core collapse scenario. In this case, a massive star (>30 solar masses) collapses to form...
    20 KB (2,210 words) - 12:44, 25 August 2024
  • known type II (core-collapse) supernova (the type II is caused by the cataclysmic explosion of the outer layers of a massive star as its core implodes). A...
    9 KB (1,169 words) - 03:00, 12 April 2024
  • Thumbnail for Supergiant
    until they develop an iron core, at which point the core collapses to produce a Type II supernova. Once these massive stars leave the main sequence, their...
    39 KB (5,371 words) - 18:49, 20 July 2024
  • Thumbnail for WR 104
    to experience a core-collapse supernova with a small chance of producing a long-duration gamma-ray burst. The possibility of a supernova explosion from...
    21 KB (2,312 words) - 04:21, 30 August 2024
  • Thumbnail for R136a1
    R136a1 (section Supernova)
    of energy in the core will cause it to collapse as a pair-instability supernova (PISN), sometimes called a pair-creation supernova (PCSN). A PISN is...
    43 KB (5,166 words) - 23:20, 22 August 2024
  • core collapses, powered by release of gravitational potential energy via neutrino emission. One model for the formation of this category of supernova...
    48 KB (5,057 words) - 04:49, 19 July 2024
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