The Near-Contact System V387 Cygni: BVRI Photometry and Modelling

Details The Near-Contact System V387 Cygni: BVRI Photometry and Modelling The Near-Contact System V387 Cygni: BVRI Photometry and Modelling

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.304...63m&link_type=abstract

Astrophysics and Space Science, Volume 304, Issue 1-4, pp. 63-65

Astronomy and Astrophysics

Astrophysics

Binaries: Eclipsing, Binaries: Near-Contact, V387 Cyg

Scientific paper

The first complete CCD BVRI-filter light curves of the eclipsing near-contact binary V387 Cyg were obtained during 5 nights in 2004 at Kryoneri Observatory, Greece. Their analysis with the W-D program indicates a semi-detached configuration with possible cool spots, although no O' Connell effect is present and a strong asymmetry after Min II can be explained assuming either a strong flare or circumstellar matter.

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