SV Cam BVR light curves in Feb. 2001 - March 2002 (Zboril, 2003)

Details SV Cam BVR light curves in Feb. 2001 - March 2002 (Zboril, 2003) SV Cam BVR light curves in Feb. 2001 - March 2002 (Zboril, 2003)

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34060193z&link_type=abstract

VizieR On-line Data Catalog: J/A+A/406/193. Originally published in: 2003A&A...406..193Z

Computer Science

Binaries: Eclipsing, Photometry

Scientific paper

We present the analysis of new BVR light curves for the active star SV Cam. The Roche model with spotted areas on the hotter primary component fits satisfactorily all filter observations yielding two spots in intermediate latitudes and covering about 1.5% each of the stellar surface. Both are ~1000K cooler than surrounding photosphere. The comparison with an earlier season (January/February 2000) suggests that the spots probably evolved in area longitude and latitude but basic and preferred orientation from previous season is confirmed.
The comparison stars were SAO 1045 (standard) and SAO 1030 (check).
(3 data files).

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