The detached eclipsing binary system GX Geminorum | Zendy

SánchezBajo F. | Zendy; GarrigósSánchez A. | Zendy; GómezForrellad J.M. | Zendy; NomenTorres J. | Zendy; Kleikamp W. | Zendy; Frank P. | Zendy; Moschner W. | Zendy; Quester W. | Zendy; GarcíaMelendo E. | Zendy

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The detached eclipsing binary system GX Geminorum

Author(s) -

SánchezBajo F.,

GarrigósSánchez A.,

GómezForrellad J.M.,

NomenTorres J.,

Kleikamp W.,

Frank P.,

Moschner W.,

Quester W.,

GarcíaMelendo E.

Publication year - 2003

Publication title -

astronomische nachrichten

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.394

H-Index - 63

eISSN - 1521-3994

pISSN - 0004-6337

DOI - 10.1002/asna.200310160

Subject(s) - subgiant , physics , astrophysics , stars , binary number , astronomy , binary star , binary system , mathematics , arithmetic , globular cluster

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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