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Light curve analysis of the late type binary V523 Cassiopeiae
Author(s) -
O. Latković,
M. Zboril,
G. Djurašević
Publication year - 2009
Publication title -
serbian astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.196
H-Index - 16
eISSN - 1820-9289
pISSN - 1450-698X
DOI - 10.2298/saj0978045l
Subject(s) - physics , light curve , contact binary , binary number , astrophysics , type (biology) , binary star , term (time) , binary system , astronomy , stars , biology , ecology , arithmetic , mathematics
We present the analysis of V and R light curves of the late type contact binary V523 Cas for the season of 2006. These observations make part of the monitoring program aimed at studying the long-term light curve variability in this system. Our results confirm that the system is in an over contact configuration, and include a bright spot in the neck region of the cooler and larger primary. We compare these results with the previous solution, obtained for the season 2005 dataset and discuss the differences

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