中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Abundance distribution in the solar system and slow neutron capture elements in AGB 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2003
卷号27期号:11页码:978-983
关键词abundance AGB s-process
通讯作者Guangxi Normal Univ, Acad Phys & Informat Engn, Guilin 541004, Peoples R China ; Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China ; Hebei Normal Univ, Dept Phys, Shijiazhuang 050016, Peoples R China ; Natl Lab Heavy Ion Accelerator Lanzhou, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China
英文摘要By re-analyzing the results of the theoretical abundance of AGB stellar models and the observed abundances of 51 AGB samples, we find that the abundance distribution of heavy elements belonging to the main-component of slow neutron capture process (SMH elements) of any AGB star is similar to that of the scaled s-process main component of the solar system. It means that superposition of the SMH element abundance distributions of AGB stars should be similar to that of the scaled solar s-main component. As a conclusion, the heavy element abundance pattern of the solar s-main component is a typical one and can be used as a standard in the investigation of heavy element abundances in single star.
学科主题Physics
类目[WOS]Physics, Nuclear ; Physics, Particles & Fields
研究领域[WOS]Physics
原文出处SCI
语种英语
WOS记录号WOS:000186635400008
源URL[http://ir.ihep.ac.cn/handle/311005/238829]  
专题高能物理研究所_理论物理室
作者单位中国科学院高能物理研究所
推荐引用方式
GB/T 7714
Zhang MJ,Zhang B,Li GL,et al. Abundance distribution in the solar system and slow neutron capture elements in AGB stars[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2003,27(11):978-983.
APA 张妙静,张波,厉光烈,Zhang, MJ,Zhang, B,&Li, GL.(2003).Abundance distribution in the solar system and slow neutron capture elements in AGB stars.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,27(11),978-983.
MLA 张妙静,et al."Abundance distribution in the solar system and slow neutron capture elements in AGB stars".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 27.11(2003):978-983.

入库方式: OAI收割

来源:高能物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。