Results 11 to 20 of about 2,475,925 (212)
The mechanism(s) of core-collapse supernovae [PDF]
Core-collapse supernovae (CCSNe) are the explosions that attend the deaths of massive stars. Despite decades of research, several aspects of the mechanism that drives these explosions remain uncertain and the subjects of continued investigation. In this short review, I will give an overview of the CCSN mechanism and current research in the field.
Sean M Couch
exaly +5 more sources
Turbulence in Core-collapse Supernovae
It is understood in a general sense that turbulent fluid motion below the shock front in a core-collapse supernova stiffens the effective equation of state of the fluid and aids in the revival of the explosion.
David Calvert +6 more
doaj +4 more sources
Magnetorotational Explosions of Core-Collapse Supernovae
Core-collapse supernovae are accompanied by formation of neutron stars. The gravitation energy is transformed into the energy of the explosion, observed as SN II, SN Ib,c type supernovae.
Gennady S. Bisnovatyi-Kogan +2 more
doaj +3 more sources
The demographics of core-collapse supernovae
Context. The observational properties of core-collapse supernovae are shaped by the envelopes of their progenitors. In massive binary systems, mass-transfer drastically alters the pre-supernova structures compared to single stars, which leads to a ...
Ercolino Andrea +5 more
doaj +2 more sources
Core-collapse supernova explosion theory [PDF]
Review article published in ...
A. Burrows, D. Vartanyan
openaire +3 more sources
Search for core-collapse supernovae using the MiniBooNE neutrino detector [PDF]
We present a search for core-collapse supernovae in the Milky Way galaxy, using the MiniBooNE neutrino detector. No evidence is found for core-collapse supernovae occurring in our Galaxy in the period from December 14, 2004 to July 31, 2008 ...
Koutsoliotas, S. +32 more
core +6 more sources
Core-collapse supernovae as cosmic ray sources. [PDF]
Core-collapse supernovae produce fast shocks which expand into the dense circumstellar medium (CSM) of the stellar progenitor. Cosmic rays (CRs) accelerated at these shocks can induce the growth of electromagnetic fluctuations in the pre-shock medium.
Marcowith A +4 more
europepmc +10 more sources
Revealing the Progenitor of SN 2021zby through Analysis of the TESS Shock-cooling Light Curve
We present early observations and analysis of the double-peaked Type IIb supernova (SN IIb) SN 2021zby. TESS captured the prominent early shock-cooling peak of SN 2021zby within the first ∼10 days after explosion with a 30 minute cadence.
Qinan Wang +43 more
doaj +1 more source
The physics of core-collapse supernovae [PDF]
Review article; 17 pages, 5 ...
Woosley, S., Janka, T.
openaire +3 more sources
The progenitors of core-collapse supernovae [PDF]
We present maps of the nature of single star progenitors of supernovae and their remnants in mass and metallicity space. We find our results are similar to others but we have gone further in varying the amount of mixing and using various mass-loss schemes to see how the maps change.
Eldridge, J. J., Tout, C. A.
openaire +2 more sources

