Abundance distribution of slow-process main heavy elements in AGB stars | |
Zhang MJ(张妙静); Shen PN(沈彭年); Liu XH(刘宪辉); Zhang, MJ; Zhang, B![]() | |
刊名 | CHINESE PHYSICS LETTERS
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2003 | |
卷号 | 20期号:6页码:962-964 |
通讯作者 | Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China ; Guangxi Normal Univ, Dept Phys & Elect Sci, Guilin 541004, Peoples R China ; Natl Lab Heavy Ion Accelerator Lanzhou, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China ; Hebei Normal Univ, Dept Phys, Shijiazhuang 050016, Peoples R China |
英文摘要 | By re-analysing the results of the theoretical abundance of asymptotic giant branch (AGB) stellar models and the observed abundances of 51 AGB samples, we find that the abundance distribution of s-process main heavy (SMH) elements of any AGB star is similar to the scaled s-process main component of the solar system. This means that superposition of the SMH element abundance distributions of AGB stars should be similar to the scaled solar s-process main component. As a conclusion, the abundance pattern of the solar SMH elements is not only an average result of a complex chemical evolution of galaxy, but also a typical one that can be used as a standard in abundance investigation. |
学科主题 | Physics |
类目[WOS] | Physics, Multidisciplinary |
研究领域[WOS] | Physics |
原文出处 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000183671800054 |
内容类型 | 期刊论文 |
源URL | [http://ir.ihep.ac.cn/handle/311005/238811] ![]() |
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,Shen PN,Liu XH,et al. Abundance distribution of slow-process main heavy elements in AGB stars[J]. CHINESE PHYSICS LETTERS,2003,20(6):962-964. |
APA | 张妙静,沈彭年,刘宪辉,Zhang, MJ,Zhang, B,&Li, GL.(2003).Abundance distribution of slow-process main heavy elements in AGB stars.CHINESE PHYSICS LETTERS,20(6),962-964. |
MLA | 张妙静,et al."Abundance distribution of slow-process main heavy elements in AGB stars".CHINESE PHYSICS LETTERS 20.6(2003):962-964. |
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