Kinematics of W UMa-type binaries

DOI

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.

Cone search capability for table J/MNRAS/357/497/WUMa (W UMa stars: identifications, astrometry, kinematics and physical parameters (tables 1, 2 and 5 of the paper))

Identifier
DOI http://doi.org/10.26093/cds/vizier.73570497
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/357/497
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/357/497
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/357/497
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/357/497
Provenance
Creator Bilir S.; Karatas Y.; Demircan O.; Eker Z.
Publisher CDS
Publication Year 2005
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Exoplanet Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy