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SNR G011.2−00.3 (categoría Restos de supernova)de agosto de 2021. Jacovich, Taylor et al. (2021). «A Grid of Core-collapse Supernova Remnant Models. I. The Effect of Wind-driven Mass Loss». The Astrophysical…7 kB (736 palabras) - 15:15 23 ene 2024
Radiación de sincrotrón (sección En supernovas)«Ejection of the Massive Hydrogen-rich Envelope Timed with the Collapse of the Stripped SN 2014C». The Astrophysical Journal 835 (2). doi:10.3847/1538-4357/835/2/140…19 kB (2157 palabras) - 09:43 15 abr 2024
Resultados de la Wikipedia en inglés.
- collapsing core of the star. The jets would also transfer energy into the expanding outer shell, producing a super-luminous supernova. Ultra-stripped…199 kB (21 759 palabras) - 02:22 5 jun 2024
- Type Ib and Ic supernovae (redirección desde Type Ib supernova)referred to as stripped core-collapse supernovae. When a supernova is observed, it can be categorized in the Minkowski–Zwicky supernova classification…13 kB (1513 palabras) - 09:38 28 ago 2023
- 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…48 kB (4780 palabras) - 23:44 16 may 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 (5069 palabras) - 19:35 18 may 2024
- 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 (2516 palabras) - 10:45 1 abr 2024
- 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 (2180 palabras) - 21:30 1 jun 2024
- Stellar evolution (sección Supernova)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 or black hole. Although…49 kB (6408 palabras) - 15:52 29 may 2024
- eventually merges with the core of the giant/supergiant; other times the infall stops before core merger. This kind of supernova has been invoked to explain…12 kB (1661 palabras) - 16:10 25 dic 2023
- variables, Wolf–Rayet stars, and the progenitors of certain classes of core collapse supernova is still disputed. Single massive stars may be unable to expel…146 kB (16 317 palabras) - 17:14 5 jun 2024
- Supergiant (sección Supernova progenitors)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 (5309 palabras) - 00:06 1 jun 2024
- 4 M☉. They result from the supernova explosion of a massive star, combined with gravitational collapse, that compresses the core past white dwarf star density…113 kB (13 659 palabras) - 16:29 5 jun 2024
- Wanajo, S.; et al. (2003). "The r-Process in Supernova Explosions from the Collapse of O-Ne-Mg Cores". The Astrophysical Journal. 593 (2): 968–979.…20 kB (2582 palabras) - 04:27 7 abr 2024
- an electron capture supernova through the collapse of an oxygen-neon core. Main-sequence stars, burning hydrogen in their cores, with masses between…33 kB (4223 palabras) - 10:03 17 may 2024
- Eta Carinae (sección Potential supernova)(SLSN) or hypernova, several times more luminous than a typical core collapse supernova and much longer-lasting. Highly massive progenitors may also eject…123 kB (14 800 palabras) - 23:53 16 mar 2024
- Helium flash (redirección desde Core Helium Flash)in the core is exhausted, some of the helium left behind is instead compacted into degenerate matter, supported against gravitational collapse by quantum…13 kB (1615 palabras) - 10:45 11 may 2024
- White dwarf (sección Type Iax supernova)degeneracy pressure. At this point the core of the star will collapse and it will explode in a core-collapse supernova which will leave behind a remnant neutron…163 kB (18 562 palabras) - 05:55 8 jun 2024
- initiate core carbon burning and even some neon burning. They form oxygen–magnesium–neon cores, which may collapse in an electron-capture supernova, or they…16 kB (2321 palabras) - 14:59 5 jun 2024
- neutron star merging with and becoming the core of another star Supernova progenitor, a star that could collapse into a black hole after the end of its life…4 kB (434 palabras) - 01:15 8 ene 2024
- Star formation (redirección desde Cloud collapse)cloud and initiate its gravitational collapse. Molecular clouds may collide with each other, or a nearby supernova explosion can be a trigger, sending…45 kB (5263 palabras) - 18:55 20 abr 2024
- WR stars are expected to experience core collapse when they have generated an iron core, and resulting supernova explosions would be of type Ib or Ic…96 kB (10 597 palabras) - 16:01 2 may 2024
- Georgy, Cyril; Ekström, Sylvia (2013). "Fundamental properties of core-collapse supernova and GRB progenitors: Predicting the look of massive stars before…38 kB (4701 palabras) - 19:40 17 feb 2024