Chromospherically active binaries Virtual Observatory Resource

Authors
  1. Karatas Y.
  2. Bilir S.
  3. Eker Z.
  4. Demircan O.
  5. Published by
    CDS
Abstract

The kinematics of 237 chromospherically active binaries (CABs) were studied. The sample is heterogeneous with different orbits and physically different components from F to M spectral-type main-sequence stars to G and K giants and supergiants. The computed U, V, W space velocities indicate that the sample is also heterogeneous in velocity space.

Keywords
  1. Spectroscopic binary stars
  2. Proper motions
  3. Radial velocity
Bibliographic source Bibcode
2004MNRAS.349.1069K
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/349/1069
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/349/1069

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/349/1069
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/349/1069
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/349/1069
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/MNRAS/349/1069/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/349/1069/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/349/1069/table1?

History

2007-08-20T15:33:38Z
Resource record created
2007-08-20T15:33:38Z
Created
2017-12-22T05:33:24Z
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