The initial-final mass relation of stars

doi:10.1016/S0275-1062(98)00006-X

YNAO OpenIR > 大样本恒星演化研究组

	The initial-final mass relation of stars
	Han ZW(韩占文)1,2
发表期刊	CHINESE ASTRONOMY AND ASTROPHYSICS
	1998-01
卷号	22 期号:1 页码:41-48
DOI	10.1016/S0275-1062(98)00006-X
产权排序	第2完成单位
收录类别	SCI
关键词	Age Stars Stellar Evolution Mass Loss White Dwarf
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.
语种	英语
学科领域	天文学 ; 恒星与银河系 ; 恒星形成与演化
文章类型	Article
ISSN	0275-1062
URL	查看原文
WOS记录号	WOS:000082336300006
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	PLANETARY-NEBULAE ; EVOLUTION ; GIANTS ; END
引用统计
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/4385
专题	大样本恒星演化研究组
通讯作者	Han ZW(韩占文)
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
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	Han ZW. The initial-final mass relation of stars[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,1998,22(1):41-48.
APA	Han ZW.(1998).The initial-final mass relation of stars.CHINESE ASTRONOMY AND ASTROPHYSICS,22(1),41-48.
MLA	Han ZW."The initial-final mass relation of stars".CHINESE ASTRONOMY AND ASTROPHYSICS 22.1(1998):41-48.

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The initial-final ma（472KB）	期刊论文	出版稿	开放获取	CC BY-NC-SA	浏览请求全文