NAOC Open IR
蓝离散星研究现状(Ⅱ):观测特性
新宇; 邓李才; 梁艳春
2006
Source Publication天文学进展
ISSN1000-8349
Volume024Issue:003Pages:223
Abstract不同恒星系统(银河系晕、疏散星团、球状星团、矮星系)中蓝离散星所表现出的观测特性各不相同,这与恒星系统动力学环境及相应的蓝离散星主导形成机制直接相关。因此,分析研究蓝离散星的不同观测特性,也就成为研究蓝离散星形成机制、恒星及双星系统演化以及恒星系统动力学演化的有效方法。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/44255
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
新宇,邓李才,梁艳春. 蓝离散星研究现状(Ⅱ):观测特性[J]. 天文学进展,2006,024(003):223.
APA 新宇,邓李才,&梁艳春.(2006).蓝离散星研究现状(Ⅱ):观测特性.天文学进展,024(003),223.
MLA 新宇,et al."蓝离散星研究现状(Ⅱ):观测特性".天文学进展 024.003(2006):223.
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