| A photometric analysis of the neglected EW-type binary V336 TrA | |
Kriwattanawong, W.1; Sarotsakulchai, T.2,3,4 ; Maungkorn, S.1; Reichart, D. E.5; Haislip, J. B.5; Kouprianov, V. V.5; LaCluyze, A. P.5; Moore, J. P.5
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| 发表期刊 | NEW ASTRONOMY
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| 2018-05-01 | |
| 卷号 | 61页码:1-4 |
| DOI | 10.1016/j.newast.2017.11.002 |
| 产权排序 | 第3完成单位 |
| 收录类别 | SCI |
| 关键词 | Stars: Binaries: Close Stars: Binaries: Eclipsing Stars: Individual (V336 Tra) |
| 摘要 | This study presents an analysis of photometric light curves and absolute parameters for the EW-type binary V336 TrA. VRI imaging observations were taken in 2013 by using the robotic telescopes PROMPT 4 and PROMPT 5 at Cerro Tololo Inter-American Observatory (CTIO), Chile. The observed light curves were fitted by using the Wilson-Devinney method. The results showed that V336 TrA is a W-type contact binary with a mass ratio of q = 1.396. The binary is a weak contact system with a fill-out factor of f = 15.69%. The system contains components with masses of 0.653 M-circle dot and 0.912 M-circle dot for the hotter and the cooler, respectively. The location of the secondary (less massive) component on the log M-log L diagram was found to be near the TAMS. The component has evolved to be oversize and overluminous. The orbital angular momentum of the binary was found to be log J(o) = 51.61 cgs, less than all detached systems for same mass. The system has undergone angular momentum and/or mass loss, during the binary evolution from the detached to contact system. |
| 资助项目 | Chiang Mai University ; NASA grant |
| 项目资助者 | Chiang Mai University ; NASA grant |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 恒星与银河系 |
| 文章类型 | Article |
| 出版者 | ELSEVIER SCIENCE BV |
| 出版地 | PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS |
| ISSN | 1384-1076 |
| URL | 查看原文 |
| WOS记录号 | WOS:000424180000001 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | ALL-SKY SURVEYS ; CONTACT BINARIES ; ECLIPSING BINARIES ; VARIABLE-STARS ; LIGHT CURVES ; EVOLUTION |
| 引用统计 | |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/12291 |
| 专题 | 双星与变星研究组 |
| 通讯作者 | Kriwattanawong, W. |
| 作者单位 | 1.Department of Physics and Materials Science, Faculty of Science, Chiang Mai University, Chiang Mai, 50200, Thailand 2.National Astronomical Research Institute of Thailand, Ministry of Science and Technology, Bangkok, Thailand 3.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, 650216 Kunming, Republic of China 4.University of Chinese Academy of Sciences, 19 A Yuquan Rd., Shijingshan District, 100049 Beijing, Republic of China 5.Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3255, USA |
| 推荐引用方式 GB/T 7714 | Kriwattanawong, W.,Sarotsakulchai, T.,Maungkorn, S.,et al. A photometric analysis of the neglected EW-type binary V336 TrA[J]. NEW ASTRONOMY,2018,61:1-4. |
| APA | Kriwattanawong, W..,Sarotsakulchai, T..,Maungkorn, S..,Reichart, D. E..,Haislip, J. B..,...&Moore, J. P..(2018).A photometric analysis of the neglected EW-type binary V336 TrA.NEW ASTRONOMY,61,1-4. |
| MLA | Kriwattanawong, W.,et al."A photometric analysis of the neglected EW-type binary V336 TrA".NEW ASTRONOMY 61(2018):1-4. |
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| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| A photometric analys（826KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | |
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