Results 111 to 120 of about 3,393,330 (216)
Context. The gravitational collapse of massive stars at the end of their lives leads to powerful supernova explosions that produce new stellar-sized compact objects, regulate the dynamics of their host galaxies, and produce new heavy elements that ...
Celati A. +4 more
doaj +1 more source
We investigate SN 2014C using three-dimensional (3D) hydrodynamic modeling, focusing on its early interaction with a dense circumstellar medium (CSM). Our objective is to uncover the pre-supernova (SN) CSM structure and constrain the progenitor star’s ...
Salvatore Orlando +11 more
doaj +1 more source
Supernovae Drive Large-scale, Incompressible Turbulence through Small-scale Instabilities
The sources of turbulence in our Galaxy may be diverse, but core-collapse supernovae (SNe) alone provide enough energy to sustain a steady-state galactic turbulence cascade at the observed velocity dispersion.
James R. Beattie
doaj +1 more source
Shell-model applications in supernova physics
This manuscript reviews recent applications of the nuclear shell-model for the calculation of several quantities relevant for the core-collapse supernova dynamics and nucleosynthesis.
G. Martınez-Pinedo
core +1 more source
The double detonation model is one of the prevalent explosion mechanisms of Type Ia supernovae (SNe Ia) wherein an outer helium shell detonation triggers a core detonation in the white dwarf (WD).
Nethra Rajavel +2 more
doaj +1 more source
Supernova Hunters Discovery of 24 Optical Transients with Pan-STARRS
Here we report the discovery of 24 transient objects as part of the Pan-STARRS Survey for Transients (PSST) found by citizen scientists involved in the Supernova Hunters Zooniverse Project.
Sim, S. +48 more
core +1 more source
Simulating molecular cloud regulated star formation in Galaxies [PDF]
This thesis is primarily concerned with understanding the process of galaxy formation via the simulation of the interstellar medium, star formation and supernova feedback.
Booth, Craig Martin
core
How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
Energy-transport effects can alter the structure that develops as a supernova evolves into a supernova remnant. The Rayleigh–Taylor instability is thought to produce structure at the interface between the stellar ejecta and the circumstellar matter ...
A. Shimony +27 more
core +1 more source
Dynamics and Nonthermal Emission of Shell Supernova Remnants / Reynolds S. // X-Ray and Radio
Supernova remnants illustrate the return of mass and energy from stars to the interstellar medium, connecting one generation of star formation with the next.
S P Reynolds
core
Dynamical Evolution and Radiative Processes of Supernova Remnants [PDF]
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

