Eclipsing binaries with candidate CP stars

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.33240137
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/324/137
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/324/137
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/324/137
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/324/137
Provenance
Creator North P.; Studer M.; Kunzli M.
Publisher CDS
Publication Year 1997
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy