BUL--SC16 335: A New Eclipsing Pre-Cataclysmic Binary with a Very Short Orbital Period
Abstract
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.
- Publication:
-
15th European Workshop on White Dwarfs
- Pub Date:
- September 2007
- Bibcode:
- 2007ASPC..372..487P