Abstract
The main goal of this work is to derive a good fit to multicolor light curves of three eclipsing binary systems containing a sdB-type star: PG1336-018, HS0705+6700 and HW Vir and to check how different temperature of the cool star could be derived for two different reflection models.
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Zola, S., Niarchos, P., Østensen, R. (2003). The Temperature of the Cool Stars in Three Eclipsing Binary Systems with The SDB Components: HW VIR, PG1336-018 and HS0705+670. In: de Martino, D., Silvotti, R., Solheim, JE., Kalytis, R. (eds) White Dwarfs. NATO Science Series, vol 105. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0215-8_30
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DOI: https://doi.org/10.1007/978-94-010-0215-8_30
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