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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Main Authors: Qian S.-B., Yang Y.-G., Soonthornthum B., Zhu L.-Y., He J.-J., Yuan J.-Z.
格式: Article
語言:English
出版: 2014
在線閱讀:http://www.scopus.com/inward/record.url?eid=2-s2.0-24144439313&partnerID=40&md5=78e74b1cd5fa4df7fd9f10bda58396fb
http://cmuir.cmu.ac.th/handle/6653943832/4971
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機構: Chiang Mai University
語言: English