中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Neutron capture elements in poor-metal stars

文献类型:期刊论文

作者Zhang MJ(张妙静); Zhang B(张波); Li GL(厉光烈); Zhang, MJ; Zhang, B; Li, GL
刊名HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
出版日期2004
卷号28期号:1页码:#REF!
关键词poor-metal neutron capture component coefficient abundance
其他题名贫金属星的中子俘获元素
通讯作者Zhang, MJ (reprint author), Guangxi Normal Univ, Coll Phys & Informat Technol, Guilin, Peoples R China.
英文摘要By means of the component coefficient equation and the updated data of abundances of the solar system, we calculate the element abundances of 64 poor-metal stars. The result shows that the rapid neutron capture process (r-process) is the main source of neutron capture elements in poor-metal stars. Besides, the yields of heavy neutron capture elements in stars whose metallicity is less than -2.5 may come from pure r-process. The producer of the heavy neutron capture elements may differ from that of the light.
学科主题Physics
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields
收录类别SCI
WOS记录号WOS:000188651300006
公开日期2016-05-03
源URL[http://ir.ihep.ac.cn/handle/311005/225616]  
专题高能物理研究所_理论物理室
推荐引用方式
GB/T 7714
Zhang MJ,Zhang B,Li GL,et al. Neutron capture elements in poor-metal stars[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2004,28(1):#REF!.
APA 张妙静,张波,厉光烈,Zhang, MJ,Zhang, B,&Li, GL.(2004).Neutron capture elements in poor-metal stars.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,28(1),#REF!.
MLA 张妙静,et al."Neutron capture elements in poor-metal stars".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 28.1(2004):#REF!.

入库方式: OAI收割

来源:高能物理研究所

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