中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
WZ And, a probable contact system with mass ratio very close to unity

文献类型:期刊论文

作者Zhang, XB; Zhang, RX
刊名NEW ASTRONOMY
出版日期2006-03-01
卷号11期号:5页码:339-343
关键词binaries eclipsing-photometry-stars individual (WZ And)
英文摘要We present B and V time-series CCD photometry of the short-period eclipsing binary WZ And. Eight new epochs of minimum light were determined from the observations covering five primary and three secondary eclipses. Refined period and new ephemeris are given for the system based on the photoelectric and CCD photometric times of minima obtained in the recent 20 years. A period study covering 100 years or nearly 59,000 orbital cycles reveals a cyclic but not periodic behavior of long-term period variations. Two major period jumps can be indicated. That could be evidence for the existence of a very eccentric third body of the eclipsing system. The light curve shows continuous light changes outside eclipses in both V and B band, indicating that it could be of EW rather EB type. A simultaneous solution of the two light curves was computed using the Wilson-Devinney code. The solution indicates that WZ And is in shallow contact with a fill-out factor of similar to 6%. A photometric mass ratio of q = 1.00 +/- 0.01 was derived for the system. Discussions on the period behavior and the probable evolutionary status of the system suggest that WZ And could very probably be a newly formed equal-mass contact system. (c) 2005 Elsevier B.V. All rights reserved.
收录类别SCI
语种英语
WOS记录号WOS:000235778300002
源URL[http://ir.bao.ac.cn/handle/114a11/7059]  
专题国家天文台_光学天文研究部
作者单位Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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GB/T 7714
Zhang, XB,Zhang, RX. WZ And, a probable contact system with mass ratio very close to unity[J]. NEW ASTRONOMY,2006,11(5):339-343.
APA Zhang, XB,&Zhang, RX.(2006).WZ And, a probable contact system with mass ratio very close to unity.NEW ASTRONOMY,11(5),339-343.
MLA Zhang, XB,et al."WZ And, a probable contact system with mass ratio very close to unity".NEW ASTRONOMY 11.5(2006):339-343.

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来源:国家天文台

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