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WASP light curve of the eclipsing binary VZ CVn

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Author(s): Latković O.

Journal: Serbian Astronomical Journal
ISSN 1450-698X

Volume: 2012;
Issue: 184;
Start page: 77;
Date: 2012;
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Keywords: binaries: eclipsing | binaries: spectroscopic | stars: individual: VZ CVn

ABSTRACT
The WASP light curve of the eclipsing binary VZ CVn, consisting of more than 14000 individual observations, is analyzed for photometric elements using the modeling code of Đurašević (1992). The spectroscopic parameters are adopted from the recent radial velocity work by Pribulla et al. (2009). The results of the study include new times of minimum light, an improved ephemeris, and the updated physical and orbital parameters of the system.
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