中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
KIC 4762887: A near-contact binary or an ellipsoidal variable star?

文献类型:期刊论文

作者Li XZ(李旭志)1,2,3,4; Liu L(刘亮)1,2,3,4
刊名NEW ASTRONOMY
出版日期2021-04-01
卷号84页码:4
关键词Stars-eclipsing binary Stars-ellipsoidal variable Individual-KIC 4762887
ISSN号1384-1076
DOI10.1016/j.newast.2020.101539
产权排序第1完成单位
文献子类Article
英文摘要

KIC 4762887 is a variable star with a very small amplitude discovered by Keplerand show the EW-type light curve. We analyzed the light curve of KIC 4762887 by using the 2015 version of the Wilson-Devinney code. The results indicated that it is not a contact binary, maybe not even an eclipsing binary. We also modelled the light curve by the Fourier analysis. The results indicated that the main effect in the light variations of KIC 4762887 is the ellipsoidal effect. Finally, we confirmed that KIC 4762887 is not an eclipsing binary, but rather an ellipsoidal variable star.

学科主题天文学 ; 恒星与银河系 ; 恒星形成与演化
URL标识查看原文
出版地RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
WOS关键词LIGHT ; KEPLER
资助项目National Natural Science Foundation of China[11773066] ; National Natural Science Foundation of China[11933008] ; young academic and technology leaders project of Yunnan Province[2015HB098] ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000600411900006
出版者ELSEVIER
资助机构National Natural Science Foundation of China[11773066, 11933008] ; young academic and technology leaders project of Yunnan Province[2015HB098] ; Open Project Program of the Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences
源URL[http://ir.ynao.ac.cn/handle/114a53/24073]  
专题云南天文台_双星与变星研究组
云南天文台_中国科学院天体结构与演化重点实验室
通讯作者Li XZ(李旭志)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences (CAS), P. O. Box 110, 650216 Kunming, P. R. China
2.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P. O. Box 110, 650216 Kunming, P. R. China
3.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, P. R. China
4.University of Chinese Academy of Sciences, Yuquan Road 19#, Sijingshang Block, 100049 Beijing, P. R. China
推荐引用方式
GB/T 7714
Li XZ,Liu L. KIC 4762887: A near-contact binary or an ellipsoidal variable star?[J]. NEW ASTRONOMY,2021,84:4.
APA Li XZ,&Liu L.(2021).KIC 4762887: A near-contact binary or an ellipsoidal variable star?.NEW ASTRONOMY,84,4.
MLA Li XZ,et al."KIC 4762887: A near-contact binary or an ellipsoidal variable star?".NEW ASTRONOMY 84(2021):4.

入库方式: OAI收割

来源:云南天文台

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