中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The initial-final mass relation of stars

文献类型:期刊论文

作者Han ZW(韩占文)1,2; Han, ZW
刊名CHINESE ASTRONOMY AND ASTROPHYSICS
出版日期1998-01
卷号22期号:1页码:41-48
关键词AGE stars stellar evolution mass loss white dwarf
ISSN号0275-1062
产权排序第二完成单位
通讯作者Han, ZW
英文摘要The author studied the relationship between the zero-age mass of a Pop I star and the mass of its degenerate core at the point in the star's evolution when the binding energy of its envelope changes from negative to positive. The relation is found to be consistent with the initial-final mass relation of Weidemann and Koester, and also agrees with the distribution of masses of planetary nebula nuclei observed by Zhang and Kwok. A similar relation is obtained for Pop II stars. The final mass for a Pop II star is greater by 10% similar to 20% than that for a Pop I star for the same initial mass.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]PLANETARY-NEBULAE ; EVOLUTION ; GIANTS ; END
收录类别SCI
原文出处http://www.sciencedirect.com/science/article/pii/S027510629800006X
语种英语
WOS记录号WOS:000082336300006
源URL[http://ir.ynao.ac.cn/handle/114a53/4385]  
专题云南天文台_大样本恒星演化研究组
通讯作者Han, ZW
作者单位1.Centre for Astrophysics, University of Sciences & Technology of China, Hefei 230026 ROC
2.Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011 ROC
推荐引用方式
GB/T 7714
Han ZW,Han, ZW. The initial-final mass relation of stars[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,1998,22(1):41-48.
APA Han ZW,&Han, ZW.(1998).The initial-final mass relation of stars.CHINESE ASTRONOMY AND ASTROPHYSICS,22(1),41-48.
MLA Han ZW,et al."The initial-final mass relation of stars".CHINESE ASTRONOMY AND ASTROPHYSICS 22.1(1998):41-48.

入库方式: OAI收割

来源:云南天文台

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