Kinematics of W UMa-type binaries Virtual Observatory Resource

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

The kinematics of 129 W Ursae Majoris type binaries (W UMas) were studied. The sample is heterogeneous with different orbits and physically different components from F to K spectral-type main-sequence stars. The computed U, V, W space velocities indicate that the sample is also heterogeneous in velocity space.

Keywords
  1. spectroscopic-binary-stars
  2. eclipsing-binary-stars
  3. proper-motions
  4. radial-velocity
Bibliographic source Bibcode
2005MNRAS.357..497B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/357/497
IVOA Identifier IVOID
ivo://CDS.VizieR/J/MNRAS/357/497
Document Object Identifer DOI
doi:10.26093/cds/vizier.73570497

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/357/497
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/357/497
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/357/497
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/357/497/WUMa?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/357/497/WUMa?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/357/497/WUMa?

History

2005-08-21T20:16:55Z
Resource record created
2005-08-21T20:16:55Z
Created
2024-06-30T20:17:14Z
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