BVRI photometry and light curve analysis of VW CEP

Details BVRI photometry and light curve analysis of VW CEP BVRI photometry and light curve analysis of VW CEP

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ap%26ss.282..645k&link_type=abstract

Astrophysics and Space Science, v. 282, Issue 4, p. 645-653 (2002).

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

Synthetic light curve solutions for the W UMa-system VW Cep have been determined by applying the most new version of Wilson (1998) approach to B-observations of 1996 and VRI-observations of 1999. From a consideration of the possible evolution of this system, it is found that the system is a partial eclipsing contact one, and its primary to be a nearly Main-Sequence F5 star of mass 0.85 Msolar and the secondary to be a dwarf of spectral type G0 of mass 0.34 Msolar.

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