Nucleation experiments on a titanium-carbon system imply nonclassical formation of presolar grains. [PDF]
Kimura Y +4 more
europepmc +1 more source
Calibration relations for core-collapse supernovae [PDF]
PUMO, MARIA LETIZIA, Zampieri L.
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Neutrinos from core-collapse supernovae
The core of a massive star (M > 8 Msun) eventually collapses. This implosion usually triggers a supernova (SN) explosion that ejects most of the stellar envelope and leaves behind a neutron star (NS) with a mass of up to about 2 Msun. Sometimes the explosion fails and a black hole forms instead.
Raffelt, Georg G. +2 more
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On Neutron Star Natal Kicks in High-mass X-Ray Binaries: Insights from Population Synthesis
The motion of neutron stars (NSs) in the Galaxy is largely dependent on natal kicks received by the NSs during supernova explosions. Thus, the measured peculiar velocities of NS high-mass X-ray binaries (HMXBs) provide valuable clues to natal kicks ...
Xiangyu Ivy Wang, Xiang-Dong Li
doaj +1 more source
The two promising scenarios to explode core collapse supernovae [PDF]
Noam Soker
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Primordial black holes could hold the key to dark matter mysteries. [PDF]
Waldrop MM.
europepmc +1 more source
Early Cosmic Evolution of Europium from Core Collapse Supernovae and/or Neutron Star Mergers [PDF]
Elisabeth Vangioni +4 more
openalex
Explosion Mechanism of Core-Collapse Supernovae --- a View Ten Years after SN 1987A [PDF]
Hans‐Thomas Janka
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Progenitors of Core-Collapse Supernovae
The progenitors of core-collapse supernovae are stars with an initial mass greater than about 8M(sun). Understanding the evolution of these stars is necessary to comprehend the evolution and differences between supernovae. We have constructed new and unique opacity tables to increase model accuracy during the latest stages of stellar evolution. We have
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The Nucleosynthesis of the Light Elements C to Al by Core Collapse Supernovae [PDF]
A. Chieffi, Marco Limongi
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