The first photometric analysis of the near-contact binary star V370 Cygni

Details The first photometric analysis of the near-contact binary star V370 Cygni The first photometric analysis of the near-contact binary star V370 Cygni

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.310..153m&link_type=abstract

Astrophysics and Space Science, Volume 310, Issue 1-2, pp. 153-157

Astronomy and Astrophysics

Astrophysics

Scientific paper

The first complete CCD light curves of the eclipsing binary system V370 Cygni have been obtained in the B, V, R and I filters during 5 consecutive nights in 2005 at Kryoneri Observatory, Greece. These curves were analyzed with the Wilson Devinney program in order to determine the geometrical and physical parameters of the system. The analysis indicates a semi-detached configuration and a mildly evolved state of the system.

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