Results 201 to 210 of about 59,386 (288)

Calibration relations for core-collapse supernovae [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
PUMO, MARIA LETIZIA, Zampieri L.
openaire   +2 more sources

Neutrinos from core-collapse supernovae

open access: yes
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
openaire   +2 more sources

On Neutron Star Natal Kicks in High-mass X-Ray Binaries: Insights from Population Synthesis

open access: yesThe Astrophysical Journal
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

Early Cosmic Evolution of Europium from Core Collapse Supernovae and/or Neutron Star Mergers [PDF]

open access: green, 2015
Elisabeth Vangioni   +4 more
openalex  

Progenitors of Core-Collapse Supernovae

open access: yes, 2005
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
openaire   +2 more sources

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