Grids of stellar models III. Virtual Observatory Resource

Authors
  1. Charbonnel C.
  2. Meynet G.
  3. Maeder A.
  4. Schaller G.
  5. Schaerer D.
  6. Published by
    CDS
Abstract

Stellar evolutionary models with mass loss and moderate overshooting at metallicity Z = 0.004 in the 0.80 to 120 M{sun} range are presented. They complete the set of grids computed with the same up-input physics for Z=0.020 and 0.001 by Schaller et al. (1992, Cat. J/A+AS/96/269), for Z=0.008 by Schaerer et al. (1992A&A...263..129S, Cat. J/A+AS/98/523) and for Z=0.040 by Schaerer et al. (1993, Cat. J/A+AS/102/339).

Keywords
  1. stellar-evolutionary-models
  2. stellar-mass-loss
  3. hertzsprung-russell-diagram
Bibliographic source Bibcode
1993A&AS..101..415C
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/101/415
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+AS/101/415

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History

2011-10-09T12:13:52Z
Resource record created
2011-10-09T12:13:52Z
Created
2017-07-11T13:09:24Z
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