IHEP OpenIR  > 理论物理室
Abundance distribution in the solar system and slow neutron capture elements in AGB stars
Zhang MJ(张妙静); Zhang B(张波); Li GL(厉光烈); Zhang, MJ; Zhang, B; Li, GL
2003
发表期刊HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
卷号27期号:11页码:978-983
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
文章类型Article
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.
关键词abundance AGB s-process
学科领域Physics
研究领域[WOS]Physics ; Physics
URL查看原文
语种英语
研究领域[WOS]Physics ; Physics
WOS类目Physics, Nuclear ; Physics, Particles & Fields
WOS记录号WOS:000186635400008
引用统计
被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/238829
专题理论物理室
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.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
5877.pdf(1071KB)期刊论文作者接受稿限制开放CC BY-NC-SA请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[张妙静]的文章
[张波]的文章
[厉光烈]的文章
百度学术
百度学术中相似的文章
[张妙静]的文章
[张波]的文章
[厉光烈]的文章
必应学术
必应学术中相似的文章
[张妙静]的文章
[张波]的文章
[厉光烈]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

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。