Supernova matter EOS Virtual Observatory Resource

Authors
  1. Buyukcizmeci N.
  2. Botvina A.S.
  3. Mishustin I.N.
  4. Published by
    CDS
Abstract

This is an introduction to the tabulated database of stellar matter properties calculated within the framework of the Statistical Model for Supernova Matter (SMSM). The tables present thermodynamical characteristics and nuclear abundances for 31 values of baryon density (10^-8^ < {rho}/{rho}_0_< 0.32, {rho}_0_= 0.15 fm^-3^ is the normal nuclear matter density), 35 values of temperature (0.2 MeV < T < 25 MeV), and 28 values of electron-to-baryon ratio (0.02 < Y_e_< 0.56). The properties of stellar matter in {beta} equilibrium are also considered. The main ingredients of the SMSM are briefly outlined, and the data structure and content of the tables are explained.

Keywords
  1. supernovae
  2. astronomical-models
  3. chemical-abundances
Bibliographic source Bibcode
2014ApJ...789...33B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/789/33
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/789/33
Document Object Identifer DOI
doi:10.26093/cds/vizier.17890033

Access

Web browser access HTML
https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/789/33
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/789/33
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/789/33
IVOA Table Access TAP
https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2017-03-13T12:55:58Z
Resource record created
2017-03-13T12:55:58Z
Created
2017-06-01T08:52:39Z
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