V407 Peg and LU Vir: Two Contact Binaries with Displaced Secondary Minima

Details V407 Peg and LU Vir: Two Contact Binaries with Displaced Secondary Minima V407 Peg and LU Vir: Two Contact Binaries with Displaced Secondary Minima

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ibvs.5991....1z&link_type=abstract

Information Bulletin on Variable Stars, 5991, 1.

Physics

2

Photometry

Scientific paper

Contact eclipsing binaries are always on circular orbit. We present two
rather unusual systems, where the secondary minimum is displaced from a
phase 0.5 from the primary one. This is probably caused by strong
asymmetry of the light curve.

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