| New Progresses on Binary Stars in Globular Cluster ω Centauri | |
Liu L(刘亮)1,2,3 ; Qian SB(钱声帮)1,2,3; Leung, Kam-Ching4; Li K(李凯)1,2,3
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| 会议录名称 | Astronomical Society of the Pacific (ASP) Conference Series - TENTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS |
| 2014-08 | |
| 卷号 | 482 |
| 页码 | 219-223 |
| 会议录编者/会议主办者 | Lee, HW; Leung, KC; Kang, YW |
| 产权排序 | 第1完成单位 |
| 收录类别 | CPCI |
| 会议名称 | 10th Pacific Rim Conference on Stellar Astrophysics |
| 会议日期 | 2013-05-27 |
| 会议地点 | Sejong University Convention Center, Seoul, Korea |
| 摘要 | Globular clusters are the oldest celestial system in the Galaxy. There is enough time to form all kinds of stars, such as, first aged stars, white dwarfs, neutron stars, even black holes. On the other hand, there should be more binary systems in the globular clusters than those in the field because of a crowded environment. Thus, we through the binaries’ light variation to research the mentioned interesting and important targets. Here, we review some new discoveries that detecting a young generation binary (NV364) and an Algol-type blue straggler (V211) in the largest globular cluster ω Centauri. |
| 资助项目 | Chinese Natural Science Foundation[11103074] ; Chinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[10973037] ; Chinese Natural Science Foundation[11203066] ; Chinese Natural Science Foundation[10903026] ; West Light Foundation of the Chinese Academy of Sciences |
| 项目资助者 | Chinese Natural Science Foundation ; West Light Foundation of the Chinese Academy of Sciences |
| 语种 | 英语 |
| 学科领域 | 天文学 ; 天体物理学 |
| 文章类型 | Proceedings Paper |
| 出版者 | ASTRONOMICAL SOC PACIFIC |
| 出版地 | 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA |
| ISBN号 | 978-1-58381-849-7; 978-1-58381-848-0 |
| URL | 查看原文 |
| 归档日期 | 2015-07-20 |
| WOS记录号 | WOS:000374279800039 |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS类目 | Astronomy & Astrophysics |
| 关键词[WOS] | Main-sequence |
| 引用统计 | |
| 文献类型 | 会议论文 |
| 条目标识符 | http://ir.ynao.ac.cn/handle/114a53/9664 |
| 专题 | 双星与变星研究组 中国科学院天体结构与演化重点实验室 |
| 通讯作者 | Liu L(刘亮) |
| 作者单位 | 1.Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, P.R. China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, P. R. China 3.Graduate University of the Chinese Academy of Sciences, 19A Yuquanlu, Sijingshang Block, 100049 Beijing, China 4.Department of Physics and Astronomy, University of Nebraska, 1400 R Street Lincoln, NE 68588, USA |
| 第一作者单位 | 中国科学院云南天文台 |
| 通讯作者单位 | 中国科学院云南天文台 |
| 推荐引用方式 GB/T 7714 | Liu L,Qian SB,Leung, Kam-Ching,et al. New Progresses on Binary Stars in Globular Cluster ω Centauri[C]//Lee, HW; Leung, KC; Kang, YW. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2014:219-223. |
| 条目包含的文件 | ||||||
| 文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
| New Progresses on Bi（102KB） | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 | ||
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