Photometric study of the eclipsing binary V396 Monocerotis

Details Photometric study of the eclipsing binary V396 Monocerotis Photometric study of the eclipsing binary V396 Monocerotis

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004an....325..661g&link_type=abstract

Astronomische Nachrichten, Vol.325, Issue 6, p.661-661

Astronomy and Astrophysics

Astronomy

1

Binaries: Close, Stars: Starspot, Stars:Individual (V396 Mon)

Scientific paper

The W UMa-type eclipsing binary V396 Mon was observed using 1m telescope of Yunnan Observatory in 2000. The new BV light curves are analyzed using Wilson-Devinney program, and the result shows that V396 Mon is a W-subtype contact binary with a mass ratio 2.94. The light curve of the system is variable, and this phenomenon probably results from starspot activity of the components.

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