NAOC Open IR
蓝离散星研究现状(Ⅰ):形成机制
新宇; 邓李才; 梁艳春
2006
Source Publication天文学进展
ISSN1000-8349
Volume024Issue:002Pages:129
Abstract大量研究表明,蓝离散星的形成可能有多种机制,目前比较流行的形成机制可以概括为以下几类:密近双星系统的质量传输及双星并合、密集星场的恒星碰撞,以及包含双星系统的恒星间(双星-单星、双星-双星)相互作用导致的恒星并合.与此同时,蓝离散星在各类恒星系统中的普遍存在,也使得研究这类恒星的形成及演化成为追踪恒星系统动力学演化、化学演化及积分光谱性质变化的有效指针.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/41517
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(Ⅰ):形成机制[J]. 天文学进展,2006,024(002):129.
APA 新宇,邓李才,&梁艳春.(2006).蓝离散星研究现状(Ⅰ):形成机制.天文学进展,024(002),129.
MLA 新宇,et al."蓝离散星研究现状(Ⅰ):形成机制".天文学进展 024.002(2006):129.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[新宇]'s Articles
[邓李才]'s Articles
[梁艳春]'s Articles
Baidu academic
Similar articles in Baidu academic
[新宇]'s Articles
[邓李才]'s Articles
[梁艳春]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[新宇]'s Articles
[邓李才]'s Articles
[梁艳春]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.