The First Photometric Analysis of the Near-Contact Eclipsing Binary V499 Cygni

Details The First Photometric Analysis of the Near-Contact Eclipsing Binary V499 Cygni The First Photometric Analysis of the Near-Contact Eclipsing Binary V499 Cygni

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confq..15m&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 15-15"

Physics

Scientific paper

The first complete CCD light curves of the eclipsing binary system V499 Cyg with an F0 primary have been obtained in the B, V, R and I filters during six nights in 2006 with the 122-cm telescope at the Kryoneri Station of the National Observatory of Athens. The light curves are analyzed with the W-D program in order to determine the geometrical and photometric elements of the system. These elements are used to derive the physical parameters of V499 Cyg and estimate its evolutionary status.

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