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Faint Core-Collapse Supernovae with Fallback
AIP Conference Proceedings, 2010A long GRB is thought to occur when a massive star ends its life and thus it is expected to be accompanied by a type Ic supernova (SN) which also results from a massive star. Several nearby long GRBs are observed with type Ic SNe. However, some nearby long GRBs are observed without SNe, even though they are close enough to be able to observe the ...
Takashi Moriya +9 more
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Nucleosynthesis in core collapse supernovae
AIP Conference Proceedings, 1995Core-collapse supernovae (CCSNe) are one of the most important nucleosynthesis sites and they hold a key role in the evolution of galaxies. In the explosion, CCSNe eject freshly synthesized iron-group nuclei from explosive burning alongside of intermediate mass elements (from hydrostatic and explosive burning), and carbon and oxygen from the pre ...
F.-K. Thielemann +2 more
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Hydrodynamics of core-collapse supernovae and their progenitors
Living Reviews in Solar Physics, 2020Bernhard Müller
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Long γ-ray bursts and core-collapse supernovae have different environments
Nature, 2006Andrew Levan, Elena Pian, Ralph Wijers
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Core-Collapse Supernovae, Neutrinos, and Gravitational Waves
Nuclear Physics, Section B, Proceedings Supplements, 2013Ernazar Abdikamalov, S Gossan
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The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae
Monthly Notices of the Royal Astronomical Society, 2020Alexander Heger +2 more
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HIGH ENERGY NEUTRINOS FROM A SLOW JET MODEL OF CORE COLLAPSE SUPERNOVAE
Modern Physics Letters A, 2005Soebur Razzaque +2 more
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