The detached eclipsing binary system GX Geminorum |
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Authors: | F. Sá nchez‐Bajo,A. Garrigó s‐Sá nchez,J.M. Gó mez‐Forrellad,J. Nomen‐Torres,W. Kleikamp,P. Frank,W. Moschner,W. Quester,E. Garcí a‐Melendo |
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Abstract: | Results of the photometric analysis by means of the Wilson‐Devinney method, combined with an empirical massradius relation for LC IV stars support the hypothesis that GX Gem is a well detached evolved system of subgiant stars. The solution is consistent with the known spectroscopic parameters obtained by Popper (1996) and the photometric data of Lacy (2002a). (© 2003 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim) |
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Keywords: | binaries: eclipsing stars: individual (GX Gem) techniques: photometric |
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