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Paper: BUL-SC16 335: A New Eclipsing Pre-Cataclysmic Binary with a Very Short Orbital Period
Volume: 372, 15th European Workshop on White Dwarfs
Page: 487
Authors: Polubek, G.; Pigulski, A.; Baran, A.; Udalski, A.
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.
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