Main sequence magnetic stars properties Virtual Observatory Resource

Authors
  1. Glagolevskij Yu.V.
  2. Published by
    CDS
Abstract

We reconsidered the previous studies of properties of magnetic stars based on the latest data on average surface magnetic fields of 177 stars. New, corrected results have been obtained that allow a better understanding of the phenomenon of magnetic chemically peculiar stars.

Keywords
  1. Peculiar variable stars
  2. Effective temperature
  3. Optical observation
  4. Catalogs
  5. Magnetic fields
  6. Apparent magnitude
  7. Astronomical models
  8. Stellar atmospheres
  9. Stellar ages
  10. Stellar radii
  11. Stellar masses
Bibliographic source Bibcode
2019AstBu..74...66G
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/AstBu/74.66
IVOA Identifier IVOID
ivo://CDS.VizieR/J/other/AstBu/74.66

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/AstBu/74.66
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/AstBu/74.66
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/AstBu/74.66
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).
IVOA Cone Search SCS
For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/other/AstBu/74.66/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/other/AstBu/74.66/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/other/AstBu/74.66/table1?

History

2019-02-11T13:23:26Z
Resource record created
2019-02-11T13:23:26Z
Created
2019-02-27T14:05:39Z
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