3 eclipsing high-mass binaries light curve Virtual Observatory Resource

Authors

1. Barr Dominguez A.
2. Chini R.
3. Haas M.
4. Pozo Nunez F.
5. Hackstein M.
6. Drass H.,Lemke R.
7. Murphy M.

Published by

CDS

Abstract

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.

Keywords

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

Bibliographic source Bibcode

2013A&A...557A..13B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/557/A13

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/557/A13

Document Object Identifer DOI

doi:10.26093/cds/vizier.35570013

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/557/A13
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/557/A13
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/557/A13

IVOA Table Access TAP

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