Contact Binaries in the Galactic Star Cluster Berkeley 39

机译：联系二进制文件在银河系中伯克利39

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The RI light curves of V6, V7 and V10 in the field of open cluster Be39 are presented and analyzed by the 2010 W-D code. The masses and radii of each component are estimated. V7 and V10 should be members of Be39 while V6 may be not a member.

机译：通过2010 W-D代码介绍和分析了开放集群BE39领域中V6，V7和V10的RI光曲线。估计每个组分的质量和半径。 V7和V10应该是BE39的成员，而V6可能不是成员。

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《Pacific Rim Conference on Stellar Astrophysics》|2014年||共5页
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作者
Liang Liu; Wenping Chen; Shengbang Qian; Liying Zhu; Jiajia He; Wenping Liao; Neelam Panwar;
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中图分类 P144-532;
关键词
Contact Binaries; Galactic Star Cluster; each component;

机译：联系二进制文件;银河系;每个组件;

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5. Dynamical evolution of stars and star clusters in the inner Galactic bulge. [D] . Kim, Sungsoo S. 2000

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Contact Binaries in the Galactic Star Cluster Berkeley 39

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