Discovery of a deep, low mass ratio overcontact binary GSC 03517-00663
Guo, Di-Fu1,2; Li, Kai1,2; Hu, Shao-Ming1; Jiang, Yun-Guo1; Gao, Dong-Yang1; Chen, Xu1
发表期刊RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2015-06
卷号15期号:6页码:889-895
DOI10.1088/1674-4527/15/6/011
收录类别SCI
关键词Stars: Binaries: Close Stars: Binaries: Eclipsing Stars: Individual (Gsc 03517-00663)
摘要

When observing blazars, we identified a new eclipsing binary named GSC 03517-00663. The light curves of GSC 03517-00663 are typical of EW-type light curves. Based on the observation using the 1 m telescope at the Weihai Observatory of Shandong University, complete VRI light curves were determined. Then, we analyzed the multiple light curves using the Wilson-Devinney program. It was found that GSC 03517-00663 has a mass ratio of q = 0.164 and a degree of contact of f = 69.2 %. GSC 03517-00663 is a deep, low mass ratio overcontact binary. The light curves of GSC 03517-00663 show a strong O'Connell effect, which was explained by employing a dark spot on the secondary component.

资助项目National Natural Science Foundation of China[11203016] ; National Natural Science Foundation of China[11333002] ; National Natural Science Foundation of China[10778619] ; National Natural Science Foundation of China[10778701] ; National Natural Science Foundation of China[U1431105] ; Natural Science Foundation of Shandong Province[ZR2012AQ008] ; Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects[OP201303]
项目资助者National Natural Science Foundation of China[11203016, 11333002, 10778619, 10778701, U1431105] ; Natural Science Foundation of Shandong Province[ZR2012AQ008] ; Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects[OP201303]
语种英语
学科领域天文学 ; 恒星与银河系 ; 恒星天文学
文章类型Article
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
出版地20A DATUN RD, CHAOYANG, BEIJING, 100012, PEOPLES R CHINA
ISSN1674-4527
URL查看原文
WOS记录号WOS:000355138900011
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]HIGH FILL-OUT ; LIGHT CURVES ; SYSTEMS ; STARS
引用统计
被引频次:4[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9373
专题中国科学院天体结构与演化重点实验室
通讯作者Li, Kai
作者单位1.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai 264209, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
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Guo, Di-Fu,Li, Kai,Hu, Shao-Ming,et al. Discovery of a deep, low mass ratio overcontact binary GSC 03517-00663[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2015,15(6):889-895.
APA Guo, Di-Fu,Li, Kai,Hu, Shao-Ming,Jiang, Yun-Guo,Gao, Dong-Yang,&Chen, Xu.(2015).Discovery of a deep, low mass ratio overcontact binary GSC 03517-00663.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,15(6),889-895.
MLA Guo, Di-Fu,et al."Discovery of a deep, low mass ratio overcontact binary GSC 03517-00663".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 15.6(2015):889-895.
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