The Short Period RS CVn Binary V1034 Herculis

Details The Short Period RS CVn Binary V1034 Herculis The Short Period RS CVn Binary V1034 Herculis

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...205.1812o&link_type=abstract

American Astronomical Society Meeting 205, #18.12; Bulletin of the American Astronomical Society, Vol. 36, p.1370

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We present new BVRI photometric observations of the eclipsing binary V1034 Her (GSC0983.1044) obtained in May 2004 with the AP7 CCD camera and 0.9-meter telescope of the Southeastern Association for Research in Astronomy (SARA), located at Kitt Peak National Observatory. In 2000 and 2001, V1034 Her was observed in V by Kaiser et al. (2002, IBVS 5231), who found the system to be an eclipsing binary with a period of about 0.815 days and with RS CVn-type light curve characteristics. We model the previously published and new light curves with the latest version of the Wilson-Devinney eclipsing binary program. For each epoch, spot parameters are obtained.

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