The First CCD BVRI Light Curves of the Near-Contact Binary V387 Cyg

Details The First CCD BVRI Light Curves of the Near-Contact Binary V387 Cyg The First CCD BVRI Light Curves of the Near-Contact Binary V387 Cyg

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ibvs.5624....1m&link_type=abstract

Information Bulletin on Variable Stars, 5624, 1.

Computer Science

Scientific paper

Complete BVRI light curves of eclipsing binary V387 Cyg show a large
asymmetry after the secondary minimum, indicative possibly of a hot and
a cool spot (although there is no observable O' Connell effect). Since a
period increase is also detected, there is strong evidence of mass
transfer.

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