Cygnus OB1-OB4 O stars radial velocities Virtual Observatory Resource

Authors
  1. Mahy L.
  2. Rauw G.
  3. De Becker M.
  4. Eenens P.
  5. Flores. C.A.
  6. Published by
    CDS
Abstract

Establishing the multiplicity of O-type stars is the first step towards accurately determining their stellar parameters. Moreover, the distribution of the orbital parameters provides observational clues to the way that O-type stars form and to the interactions during their evolution. Our objective is to constrain the multiplicity of a sample of O-type stars belonging to poorly investigated OB associations in the Cygnus complex and for the first time to provide orbital parameters for binaries identified in our sample. Such information is relevant to addressing the issue of the binarity in the context of O-type star formation scenarios.

Keywords
  1. stellar-associations
  2. o-stars
  3. radial-velocity
Bibliographic source Bibcode
2013A&A...550A..27M
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/550/A27
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/550/A27
Document Object Identifer DOI
doi:10.26093/cds/vizier.35500027

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/550/A27
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/550/A27
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/550/A27
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/A+A/550/A27/stars?
https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/550/A27/stars?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/550/A27/stars?

History

2013-01-18T09:42:35Z
Resource record created
2013-01-18T09:42:35Z
Created
2017-12-07T07:26:46Z
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