中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Absolute parameters and physical nature of two W-UMa type binaries: V1123 Tau and V1128 Tau

文献类型:期刊论文

作者Zhang, Xiao-Bin1; Ren, An-Bin1,2; Luo, Chang-Qing3; Luo, Yang-Ping3
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2011-05-01
卷号11期号:5页码:583-593
关键词binaries: eclipsing stars: late-type stars: activity stars: individual (V1123 Tau, V1128 Tau)
英文摘要We present high-precision, multi-band CCD photometry of two less-studied close binaries V1123 Tau and V1128 Tau. Complete covered light curves and a number of new times of light minima of the two eclipsing systems were obtained, based on which, revised orbital elements and new ephemerides were given. By adopting the Wilson-Devinney method, the light curves were analyzed. The photometric solutions confirm the W UMa-type nature of the binary systems. With the less-massive secondary slightly cooler than the primary, V1123 Tau could be classified as an A-type contact system. While V1128 Tau is typically considered a W-type W UMa star, the surface temperature of its secondary component is determined to be absolutely higher than the primary by about 270 K. Combining with the results of radial-velocity solutions, we determined absolute parameters of the two systems. The mass, radius and luminosity for each component of V1123 Tau were derived as: 1.36 +/- 0.05M(circle dot), 1.37 +/- 0.02R(circle dot), and 2.01 +/- 0.07L(circle dot) and 0.40 +/- 0.02M(circle dot), 0.80 +/- 0.01R(circle dot), and 0.67 +/- 0.04L(circle dot), respectively. For V1128 Tau, the absolute parameters were computed to be 1.09 +/- 0.03M(circle dot), 1.01 +/- 0.01R(circle dot), and 1.34 +/- 0.06L(circle dot) and 0.58 +/- 0.01M(circle dot), 0.76 +/- 0.01R(circle dot), and 0.91 +/- 0.05L(circle dot), respectively. Based on these results, the evolutionary status and the physical nature of the two binary systems are discussed, while also connecting with the theoretical models.
收录类别SCI
语种英语
WOS记录号WOS:000290844200008
源URL[http://ir.bao.ac.cn/handle/114a11/7989]  
专题国家天文台_光学天文研究部
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.China W Normal Univ, Inst Theoret Phys, Nanchong 637002, Peoples R China
3.Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China
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Zhang, Xiao-Bin,Ren, An-Bin,Luo, Chang-Qing,et al. Absolute parameters and physical nature of two W-UMa type binaries: V1123 Tau and V1128 Tau[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2011,11(5):583-593.
APA Zhang, Xiao-Bin,Ren, An-Bin,Luo, Chang-Qing,&Luo, Yang-Ping.(2011).Absolute parameters and physical nature of two W-UMa type binaries: V1123 Tau and V1128 Tau.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,11(5),583-593.
MLA Zhang, Xiao-Bin,et al."Absolute parameters and physical nature of two W-UMa type binaries: V1123 Tau and V1128 Tau".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 11.5(2011):583-593.

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来源:国家天文台

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