Eclipsing binaries with candidate CP stars Virtual Observatory Resource

Authors

1. North P.
2. Studer M.
3. Kunzli M.

Published by

CDS

Abstract

Photometry in the Geneva systems and radial velocities are used to determine the fundamental parameters of three eclipsing binaries, two of which having been classified as chemically peculiar and the third having relatively narrow lines. For a description of the Geneva photometric system, see e.g. <GCPD/13>

Keywords

1. eclipsing-binary-stars
2. spectroscopic-binary-stars
3. visible-astronomy
4. narrow-band-photometry

Bibliographic source Bibcode

1997A&A...324..137N

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/324/137

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/324/137

Document Object Identifer DOI

doi:10.26093/cds/vizier.33240137

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/324/137
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/324/137
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/324/137

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).