Nucleosynthesis of Elements in Evolution Processes of Asymptotic Giant Branch Stars

ZHANG Miao-jing; ZHANG Bo; LI Guang-lie

doi:10.11804/NuclPhysRev.19.03.321

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Volume 19 Issue 3

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Article Navigation > Nuclear Physics Review > 2002 > 19(3): 321-328

ZHANG Miao-jing, ZHANG Bo, LI Guang-lie. Nucleosynthesis of Elements in Evolution Processes of Asymptotic Giant Branch Stars[J]. Nuclear Physics Review, 2002, 19(3): 321-328. doi: 10.11804/NuclPhysRev.19.03.321

Citation:

ZHANG Miao-jing, ZHANG Bo, LI Guang-lie. Nucleosynthesis of Elements in Evolution Processes of Asymptotic Giant Branch Stars[J]. Nuclear Physics Review, 2002, 19(3): 321-328. doi: 10.11804/NuclPhysRev.19.03.321

Nucleosynthesis of Elements in Evolution Processes of Asymptotic Giant Branch Stars

doi: 10.11804/NuclPhysRev.19.03.321

(1 Institute of High Energy Physics; Chinese Academy of Sciences; Beijing 100039; China; 2 Department of Physics; Hebei Normal University; Shijiazhuang 050016;

Received Date: 1900-01-01
Rev Recd Date: 1900-01-01
Publish Date: 2002-09-20

Abstract

The development of nucleosynthesis theory in Asymptotic Giant Branch (AGB) stars is reviewed. Particularly, the slow neutron capture processes (s processes) and the evolution of AGB stars are briefly described.
- asymptotic giant branch star,
- stellar evolution,
- slow neutron capture process
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通讯作者: 陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

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