AAS 205th Meeting, 9-13 January 2005
Session 18 Eclipsing Binaries and Contact Binaries
Poster, Monday, January 10, 2005, 9:20am-6:30pm, Exhibit Hall

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[18.12] The Short Period RS CVn Binary V1034 Herculis

J. Ordway, W. Van Hamme (Florida International University)

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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Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.