3 eclipsing high-mass binaries light curve

DOI

We present the first results of a comprehensive photometric O-star survey performed with a robotic twin refractor at the Universitatssternwarte Bochum located near Cerro Armazones in Chile. For three high-mass stars, Pismis 24-1, CPD-51 8946, and HD 319702, we determined the period through the Lafler-Kinman algorithm and modelled the light curves within the framework of the Roche geometry.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35570013
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/557/A13
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/557/A13
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/557/A13
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/557/A13
Provenance
Creator Barr Dominguez A.; Chini R.; Haas M.; Pozo Nunez F.; Hackstein M.; Drass H.,Lemke R.; Murphy M.
Publisher CDS
Publication Year 2013
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