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; Zhang, B; Li, GL
刊名HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
出版日期2004-01
卷号28页码:30-36
关键词poor-metal neutron capture component coefficient abundance
ISSN号0254-3052
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.
WOS关键词SPECTROSCOPIC ANALYSIS ; ABUNDANCES ; MODEL
WOS研究方向Physics
语种中文
WOS记录号WOS:000188651300006
出版者SCIENCE CHINA PRESS
源URL[http://119.78.100.186/handle/113462/57150]  
专题中国科学院近代物理研究所
通讯作者Zhang, MJ
作者单位1.Guangxi Normal Univ, Coll Phys & Informat Technol, Guilin, Peoples R China
2.Natl Lab Heavy Ion Accelerator Lanzhou, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China
3.Hebei Normal Univ, Dept Phys, Shijiazhuang 050016, Peoples R China
4.Acad Sinica, Inst High Energy Phys, Beijing 100039, Peoples R China
推荐引用方式
GB/T 7714
Zhang, MJ,Zhang, B,Li, GL. Neutron capture elements in poor-metal stars[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2004,28:30-36.
APA Zhang, MJ,Zhang, B,&Li, GL.(2004).Neutron capture elements in poor-metal stars.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,28,30-36.
MLA Zhang, MJ,et al."Neutron capture elements in poor-metal stars".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 28(2004):30-36.

入库方式: OAI收割

来源:近代物理研究所

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