Mean magnetic field modulus of Ap stars Virtual Observatory Resource

Authors
  1. Mathys G.
  2. Hubrig S.
  3. Landstreet J.D.
  4. Lanz T.
  5. Manfroid J.
  6. Published by
    CDS
Abstract

The paper reports about a systematic study of the mean magnetic field modulus of Ap stars with magnetically resolved split lines. Tables 2a and 2b present the main properties of all such stars presently known. The results about their mean magnetic field modulus derived in this study are summarized in Table 3, while the individual field measurements are given in Table 4.

Keywords
  1. ap-stars
  2. magnetic-fields
Bibliographic source Bibcode
1997A&AS..123..353M
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/123/353
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+AS/123/353

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/123/353
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/123/353
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/123/353
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

1998-09-05T19:47:15Z
Resource record created
1998-09-05T19:47:15Z
Created
2019-02-27T14:01:45Z
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