Two W-subtype contact binaries: GQ Boo and V1367 Tau
文献类型：期刊论文
| 作者 | Zhang J(张嘉)1,2 ; Qian SB(钱声帮)1,2; Han ZT(韩忠涛)1,2; Wu, Yue3
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| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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| 出版日期 | 2017-04-01 |
| 卷号 | 466期号:1页码:1118-1126 |
| 关键词 | techniques: photometric binaries: eclipsing stars: evolution |
| ISSN号 | 0035-8711 |
| 产权排序 | 第1完成单位 |
| 通讯作者 | Zhang, Jia(Chinese Acad Sci, Yunnan Observ, Kunming 650216, Peoples R China) |
| 英文摘要 | Two contact binaries, GQ Boo and V1367 Tau, were observed and analysed with a new method to obtain the absolute parameters. The light-curve analysis shows that both of them are obvious W-subtype contact binaries, with much more massive but apparently cooler components (M-2/M-1 similar or equal to 2 and 4, T-2/T-1 similar or equal to 0.95 and 0.94). The orbital periods were studied using the O-C diagrams, and it is thought that the minima timings were heavily affected by the long-standing magnetic activities on the star surface, so the minima timings cannot represent the real period changes. The mass-radius relationships were proposed by the light-curve analysis alone, which is equivalent to the mean density. The density and temperature can determine the other absolute parameters in most of the time. With the almost complete star parameter space provided by PARSEC, approximate masses and radii were obtained (0.52 +/- 0.08M(circle dot) and 1.01 +/- 0.15M(circle dot) for GQ Boo, and 0.22 +/- 0.01M(circle dot) and 0.92 +/- 0.06M(circle dot) for V1367 Tau). The mass-radius relationship is a neglected useful tool to calculate the mass and radius, especially for the detached binaries. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | 天文学 |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | URSAE MAJORIS SYSTEMS ; STAR LIGHT CURVES ; ECLIPSING BINARIES ; RZ-COMAE ; VELOCITY CURVES ; AH-CANCRI ; AM LEONIS ; PARAMETERS ; PERIOD ; CALIBRATIONS |
| 收录类别 | SCI |
| 原文出处 | https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stw3153 |
| 语种 | 英语 |
| WOS记录号 | WOS:000398112400077 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/10016]  |
| 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 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China 2.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650216, China 3.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China |
| 推荐引用方式 GB/T 7714 | Zhang J,Qian SB,Han ZT,et al. Two W-subtype contact binaries: GQ Boo and V1367 Tau[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,466(1):1118-1126. |
| APA | Zhang J,Qian SB,Han ZT,&Wu, Yue.(2017).Two W-subtype contact binaries: GQ Boo and V1367 Tau.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,466(1),1118-1126. |
| MLA | Zhang J,et al."Two W-subtype contact binaries: GQ Boo and V1367 Tau".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 466.1(2017):1118-1126. |
入库方式： OAI收割
来源：云南天文台
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