Simulations of supernova explosions Virtual Observatory Resource

Authors
  1. Dessart L.
  2. Livne E.
  3. Waldman R.
  4. Published by
    CDS
Abstract

We present radiation-hydrodynamic simulations of core-collapse supernova (SN) explosions, artificially generated by driving a piston at the base of the envelope of a rotating or non-rotating red-supergiant progenitor star. We search for trends in ejecta kinematics in the resulting Type II-Plateau (II-P) SN, exploring dependencies with explosion energy and pre-SN stellar-evolution model.

Keywords
  1. supernovae
  2. astronomical-models
  3. stellar-atmospheres
Bibliographic source Bibcode
2010MNRAS.408..827D
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/408/827
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/408/827
Document Object Identifer DOI
doi:10.26093/cds/vizier.74080827

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/408/827
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/408/827
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/408/827
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2011-06-03T16:07:57Z
Resource record created
2011-06-03T16:07:57Z
Created
2024-07-12T20:14:49Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr