The s-Process Nucleosynthesis in Extremely Metal-Poor Stars as the Generating Mechanism of Carbon Enhanced Metal-Poor Stars-Reference-Cited by-同舟云学术

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The s-Process Nucleosynthesis in Extremely Metal-Poor Stars as the Generating Mechanism of Carbon Enhanced Metal-Poor Stars

Published:2017-02-27 Issue: Volume: Page:
ISSN:
Container-title:Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)
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Author:

Suda Takuma¹,Yamada Shimako²,Fujimoto Masayuki Y.³

Affiliation:

1. Research Center for the Early Universe, The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan

2. Department of Cosmosciences, Hokkaido University, Sapporo 060-0810, Japan

3. Faculty of Engineering, Hokkai-Gakuen University, Sapporo 064-0926, Japan

Publisher

Journal of the Physical Society of Japan

Link

http://journals.jps.jp/doi/pdf/10.7566/JPSCP.14.010901

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Are Faint Supernovae Responsible for Carbon-enhanced Metal-poor Stars?;The Astrophysical Journal;2020-02-12

2. Primordial to extremely metal-poor AGB and Super-AGB stars: White dwarf or supernova progenitors?;Publications of the Astronomical Society of Australia;2018

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