Results 51 to 60 of about 59,386 (288)

The First Two Years of FLEET: An Active Search for Superluminous Supernovae

open access: yesThe Astrophysical Journal, 2023
In 2019 November, we began operating Finding Luminous and Exotic Extragalactic Transients (FLEET), a machine-learning algorithm designed to photometrically identify Type I superluminous supernovae (SLSNe) in transient alert streams.
Sebastian Gomez   +7 more
doaj   +1 more source

Core-collapse supernovae: Reflections and directions [PDF]

open access: yesProgress of Theoretical and Experimental Physics, 2012
36 pages, 20 figures (43 eps files); submitted to Progress of Theoretical and Experimental Physics (PTEP)
H.-T. Janka   +5 more
openaire   +3 more sources

Effects of Symmetry Energy on the Equation of State for Simulations of Core-collapse Supernovae and Neutron-star Mergers [PDF]

open access: yesAstrophysical Journal, 2020
We construct a new equation of state (EOS) for numerical simulations of core-collapse supernovae and neutron-star mergers based on an extended relativistic mean-field model with a small symmetry energy slope L, which is compatible with both experimental ...
Hong Shen   +3 more
semanticscholar   +1 more source

Relativistic Jets in Core-collapse Supernovae [PDF]

open access: yesThe Astrophysical Journal Letters, 2019
Abstract After decades of extensive research the mechanism driving core-collapse supernovae (CCSNe) is still unclear. One common mechanism is a neutrino-driven outflow, but others have been proposed. Among those, a long-standing idea is that jets play an important role in supernova (SN) explosions. Gamma-ray bursts (GRBs) that accompany “
Tsvi Piran   +3 more
openaire   +4 more sources

The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae [PDF]

open access: yesAstrophysical Journal Supplement Series, 2020
Several thousand core-collapse supernovae (CCSNe) of different flavors have been discovered so far. However, identifying their progenitors has remained an outstanding open question in astrophysics.
S. Schulze   +56 more
semanticscholar   +1 more source

Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf

open access: yesThe Astrophysical Journal Letters, 2023
Stellar evolution theory predicts multiple pathways to the explosive deaths of stars as supernovae. Locating and characterizing the progenitors of well-studied supernovae is important to constrain the theory and to justify and design future surveys to ...
Joanne L Pledger, Michael M Shara
doaj   +1 more source

A low energy core-collapse supernova without a hydrogen envelope [PDF]

open access: yes, 2009
The final fate of massive stars depends on many factors, including mass, rotation rate, magnetic fields and metallicity. Theory suggests that some massive stars (initially greater than 25-30 solar masses) end up as Wolf-Rayet stars which are deficient in
A Filippenko   +43 more
core   +2 more sources

The Physics of Core-Collapse Supernovae: Explosion Mechanism and Explosive Nucleosynthesis [PDF]

open access: yesUniverse
Recent developments in multi-dimensional simulations of core-collapse supernovae have considerably improved our understanding of this complex phenomenon.
L. Boccioli, L. Roberti
semanticscholar   +1 more source

The Sun and core-collapse supernovae are leading probes of the neutrino lifetime [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics
The large distances travelled by neutrinos emitted from the Sun and core-collapse supernovae together with the characteristic energy of such neutrinos provide ideal conditions to probe their lifetime, when the decay products evade detection.
P. Mart'inez-Mirav'e   +2 more
semanticscholar   +1 more source

Type Ic core-collapse supernova explosions evolved from very massive stars [PDF]

open access: yes, 2013
We investigate the possibility of a super-luminous Type Ic core-collapse supernovae producing a large amount of 56Ni. Very massive stars with a main-sequence mass larger than 100 Msun and a metallicity 0.001 < Z < 0.004 are expected to explode as super ...
Okita, Shinpei   +2 more
core   +2 more sources

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