NSVS 0165 3195 Ser: A New Low-Mass Binary

Details NSVS 0165 3195 Ser: A New Low-Mass Binary NSVS 0165 3195 Ser: A New Low-Mass Binary

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..435..441w&link_type=abstract

Binaries - Key to Comprehension of the Universe. Proceedings of a conference held June 8-12, 2009 in Brno, Czech Republic. Edite

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In this paper we present a short study of newly discovered low mass eclipsing binary NSVS 1065 3195 based on our new photometric observations. Most of determinations of the fundamental parameters of low-mass stars using eclipsing binaries indicate a strong discrepancy between theory and observations. The measurements clearly indicate that the observed radii are generally larger than the predictions by stellar models. On the other hand the observed temperatures are lower than those predicted by the current models.

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