Deep, low mass ratio overcontact binary systems. III. CU Tauri and TV Muscae

Deep, low mass ratio overcontact binary systems. III. CU Tauri and TV Muscae

New CCD photometric light curves in the B and V bands of the neglected W UMa-type eclipsing variable star CU Tauri are presented. The O'Connell effect in the V light curve obtained in 2001 by Yang and Liu was about Δ V = +0.015, but it vanished in our 2004 observations. The variations in the le...

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書目詳細資料
Main Authors:	S. B. Qian, Y. G. Yang, B. Soonthornthum, L. Y. Zhu, J. J. He, J. Z. Yuan
格式:	雜誌
出版:	2018
主題:	Earth and Planetary Sciences Physics and Astronomy
在線閱讀:	https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=24144439313&origin=inward http://cmuir.cmu.ac.th/jspui/handle/6653943832/62176
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