Absolute parameters and physical nature of two W-UMa type binaries: V1123 Tau and V1128 Tau | |
Zhang, XB1; Ren, AB1,2; Luo CQ(罗常青)3; Luo YP(罗杨平)3 | |
刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2011-05 | |
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) |
ISSN号 | 1674-4527 |
通讯作者 | Zhang, XB (reprint author), Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China. |
产权排序 | 第三完成单位 |
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. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | LIGHT CURVES ; STAR LIGHT ; PHOTOMETRY ; VELOCITY ; SYSTEMS |
收录类别 | SCI |
原文出处 | http://iopscience.iop.org/article/10.1088/1674-4527/11/5/008/meta |
语种 | 英语 |
WOS记录号 | WOS:000290844200008 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5208] |
专题 | 云南天文台_恒星物理研究组 |
作者单位 | 1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 2.Institute of Theoretical Physics, China West Normal University, Nanchong 637002, China 3.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China |
推荐引用方式 GB/T 7714 | Zhang, XB,Ren, AB,Luo CQ,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, XB,Ren, AB,Luo CQ,&Luo YP.(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, XB,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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