BUL--SC16 335: A New Eclipsing Pre-Cataclysmic Binary with a Very Short Orbital Period

Details BUL--SC16 335: A New Eclipsing Pre-Cataclysmic Binary with a Very Short Orbital Period BUL--SC16 335: A New Eclipsing Pre-Cataclysmic Binary with a Very Short Orbital Period

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..372..487p&link_type=abstract

15th European Workshop on White Dwarfs ASP Conference Series, Vol. 372, proceedings of the conference held 7-11 August, 2006 in

Astronomy and Astrophysics

Astronomy

11

Scientific paper

We report the discovery of an eclipsing binary system with a very short orbital period equal to 3.0012067 h. The light curve shows very strong reflection effect and resembles light curves of binaries consisting of a hot subdwarf and late-type main-sequence star. From the analysis of the light curves we argue that the system's primary is very likely a hot subdwarf and derive preliminary parameters of the components.

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