中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Photometric solution and period analysis of the contact binary system AH Cnc

文献类型:期刊论文

作者Peng, Ying-Jiang1; Luo, Zhi-Quan1; Zhang, Xiao-Bin2; Deng, Li-Cai2; Wang, Kun2; Tian, Jian-Feng2; Yan, Zheng-Zhou2; Pan, Yang1; Fang, Wei-Jing1; Feng, Zhong-Wen4
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2016-10-01
卷号16期号:10页码:157-U70
关键词methods: data analysis astronomical instrumentation binaries: eclipsing stars, close stars Galaxy: open clusters and associations: individual (M67)
英文摘要Photometric observations of AH Cnc, a W UMa-type system in the open cluster M67, were carried out by using the 50BiN telescope. About 100 h of time-series B- and V-band data were taken, based on which eight new times of light minima were determined. By applying the Wilson-Devinney method, the light curves were modeled and a revised photometric solution of the binary system was derived. We confirmed that AH Cnc is a deep contact (f = 51%), low mass-ratio (q = 0.156) system. Adopting the distance modulus derived from study of the host cluster, we have re-calculated the physical parameters of the binary system, namely the masses and radii. The masses and radii of the two components were estimated to be respectively 1.188(+/- 0.061) M-circle dot, 1.332(+/- 0.063) R-circle dot for the primary component and 0.185(+/- 0.032) M-circle dot, 0.592(+/- 0.051) R-circle dot for the secondary. By adding the newly derived minimum timings to all the available data, the period variations of AH Cnc were studied. This shows that the orbital period of the binary is continuously increasing at a rate of dp/dt = 4.29 x 10(-10) d yr(-1). In addition to the long-term period increase, a cyclic variation with a period of 35.26 yr was determined, which could be attributed to an unresolved tertiary component of the system.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]OPEN CLUSTER M67 ; BLUE STRAGGLERS ; DEEP ; CANCRI ; STARS
收录类别SCI
语种英语
WOS记录号WOS:000385996000008
源URL[http://ir.bao.ac.cn/handle/114a11/6905]  
专题国家天文台_光学天文研究部
作者单位1.China West Normal Univ, Phys & Space Sci Coll, Nanchong 637002, Peoples R China
2.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
3.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
4.Univ Elect Sci & Technol China, Sch Phys Elect, Chengdu 610054, Peoples R China
推荐引用方式
GB/T 7714
Peng, Ying-Jiang,Luo, Zhi-Quan,Zhang, Xiao-Bin,et al. Photometric solution and period analysis of the contact binary system AH Cnc[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2016,16(10):157-U70.
APA Peng, Ying-Jiang.,Luo, Zhi-Quan.,Zhang, Xiao-Bin.,Deng, Li-Cai.,Wang, Kun.,...&Deng Licai.(2016).Photometric solution and period analysis of the contact binary system AH Cnc.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,16(10),157-U70.
MLA Peng, Ying-Jiang,et al."Photometric solution and period analysis of the contact binary system AH Cnc".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 16.10(2016):157-U70.

入库方式: OAI收割

来源:国家天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。