Results 121 to 130 of about 2,169 (225)
Magnetic Reconnection Detonation in Supernova Remnants
, 2018 Expansion of supernova remnants (SNRs) is a key process that refreshes the interstellar medium (ISM) in which a new generation of stars is born. The dynamics and radiative properties of the SNR expansion front not only reflect the physical environment of
Law, Chung K, Gao, Y, Zhang, H
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Dynamical Evolution and Radiative Processes of Supernova Remnants [PDF]
, 2016 I outline the dynamical evolution of the shell remnants of supernovae (SNRs), from initial interaction of supernova ejecta with circumstellar material (CSM) through to the final dissolution of the remnant into the interstellar medium (ISM). Supernova ejecta drive a blast wave through any CSM from the progenitor system; as material is swept up, a ...
openaire +2 more sources
Relativistic hydrodynamics simulations of supernova explosions within extragalactic jets
Context. Jets in active galactic nuclei (AGN) have to cross significant distances within their host galaxies, meeting large numbers of stars of different masses and evolution stages on their paths.
M. Perucho +4 more
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, 2017 Radiative shocks and blast waves are important in many astrophysical contexts, such as supernova remnant formation, cosmic ray production, and gamma ray bursts.
Riley, Nathan James
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Do Type Ia Supernovae Explode inside Planetary Nebulae?
The Astrophysical JournalThe nature of Type Ia supernova (SN Ia) explosions remains an open issue, with several contending progenitor scenarios actively being considered. One such scenario involves an SN Ia explosion inside a planetary nebula (PN) in the aftermath of a stellar ...
Travis Court +5 more
doaj +1 more source
, 2009 O objetivo desta dissertação foi estudar os sinais que neutrinos provenientes de supernovas galáticas poderão produzir em detectores futuros, através de simulações de eventos observados na Terra por um detector Cherenkov pela reação de decaimento beta ...
Felix, Regina Celia Medeiros +1 more
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The Astrophysical JournalCentral compact objects (CCOs) are a subclass of neutron stars (NSs) with a dipole magnetic field strength considerably weaker than those of radio pulsars and magnetars.
Akihiro Inoue +4 more
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Fine-tuned Supernova or Failed Explosion? Decoding the Origins of the G3425 Binary
The Astrophysical Journal LettersA binary system (G3425) consisting of a massive unseen component and a red giant star on a nearly circular orbit was recently discovered. The formation of such a system is puzzling because orbital stability generally breaks down due to the large mass ...
Zsolt Regály +2 more
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The Astrophysical JournalA hadron–quark phase transition (PT) may trigger supernova explosions during stellar core collapse. However, both success and failure have occurred in previous attempts to explode dying stars via this mechanism.
Xu-Run Huang +4 more
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Simulated 3D 56Ni Distributions of Type IIp Supernovae
The Astrophysical JournalWe present the first three-dimensional study of the asymptotic ejecta distributions for a suite of theoretical Type IIp supernovae originating from red supergiant (RSG) progenitors.
David Vartanyan +6 more
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