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Photometric study of W UMa type binaries in the intermediate open cluster NGC 7789

Photometric study of W UMa type binaries in the intermediate open cluster NGC 7789

作     者:Kandulapati Sriram Pasagada Vivekananda Rao 

作者机构:Department of Astronomy Osmania University 

出 版 物:《Research in Astronomy and Astrophysics》 (天文和天体物理学研究(英文版))

年 卷 期:2010年第10卷第2期

页      面:159-165页

核心收录:

学科分类:0709[理学-地质学] 07[理学] 0708[理学-地球物理学] 070401[理学-天体物理] 0825[工学-航空宇航科学与技术] 0704[理学-天文学] 

基  金:UGC 

主  题:binaries: eclipsing  binaries: close 

摘      要:The light curve solutions of two W UMa binary systems in the intermediate open cluster NGC 7789 are presented in this paper. These variables were observed using the 2 m telescope of the IUCAA-Girawali Observatory. The V passband photo- metric solutions of the two W UMa binaries were obtained using the latest version of the W-D program. The result shows that both systems are H-subtype W UMa binaries with high mass ratios.

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