W UMa-type systems in globular clusters | |
Li LF(李立芳)![]() ![]() ![]() | |
会议录名称 | IAU Symposium Proceedings Series - STAR CLUSTERS: BASIC GALACTIC BUILDING BLOCKS THROUGHOUT TIME AND SPACE |
2010 | |
卷号 | 5 |
期号 | 266 |
页码 | 451-453 |
DOI | 10.1017/S1743921309991670 |
会议录编者/会议主办者 | DeGrijs, R; Lepine, JRD |
产权排序 | 第1完成单位 |
收录类别 | CPCI |
会议名称 | 266th Symposium of the International-Astronomical-Union |
会议日期 | 2009-08-10 |
会议地点 | Rio de Janeiro, BRAZIL |
会议赞助商 | IAU Div; IAU Commiss; Int Astronom Union |
关键词 | Binaries: Eclipsing Globular Clusters: General |
摘要 | W UMa systems can be found everywhere in the Galaxy. They can be used as a distance tracer. Therefore, W UMa systems are very important to investigate the structure of the Galaxy. The distance to W UMa systems in globular clusters (GCs) is determined using a period color luminosity relation. It is found that the mean distance (r(a)) of W UMa systems is consistent with their host cluster distances (r(GC)) deduced from their intrinsic distance moduli if r(GC) <= 10 kpc. There is a significant difference between r(a) and r(GC) for r(GC) 10 >= kpc. We discuss the reasons causing this deviation. |
资助项目 | Chinese Natural Science Foundation[10673029] ; Chinese Natural Science Foundation[10773026] ; Chinese Natural Science Foundation[10821061] ; Chinese Natural Science Foundation[10521001] ; Chinese Natural Science Foundation[2007CB815406] ; Yunnan Natural Science Foundation[2007A113M] |
项目资助者 | Chinese Natural Science Foundation ; Yunnan Natural Science Foundation |
语种 | 英语 |
学科领域 | 天文学 ; 天体物理学 ; 恒星与银河系 |
文章类型 | Proceedings Paper |
出版者 | CAMBRIDGE UNIV PRESS |
出版地 | THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND |
ISBN号 | 978-0-521-76499-5 |
ISSN号 | 1743-9213 |
URL | 查看原文 |
归档日期 | 2010-07-13 |
WOS记录号 | WOS:000282782600088 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | Variable-stars ; Metal-rich ; Binary Stars ; Wuma-type ; Photometry ; Ngc-3201 ; Ngc-6397 ; Field |
引用统计 | |
文献类型 | 会议论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/251 |
专题 | 大样本恒星演化研究组 |
通讯作者 | Li LF(李立芳) |
作者单位 | National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P.O. Box 110, Kunming, Yunnan Province, 650011, P. R. China |
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 | Li LF,Zhang FH,Han ZW. W UMa-type systems in globular clusters[C]//DeGrijs, R; Lepine, JRD. THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND:CAMBRIDGE UNIV PRESS,2010:451-453. |
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 | ||
W UMa-type systems i(73KB) | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论