| s-过程和r-过程核素双超丰恒星的形成 |
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| 引用本文： | 刘清华. s-过程和r-过程核素双超丰恒星的形成[J]. 甘肃联合大学学报(自然科学版), 2011, 25(3): 37-39 |
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| 作者姓名： | 刘清华 |
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| 作者单位： | 邢台学院,物理系,河北,邢台,054001 |
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| 摘 要： | 慢中子俘获和快中子俘获过程核素双超丰的恒星,是先经历AGB星污染,再经历超新星爆发形成的,分析双超丰贫金属星HE 1305-0007可证实这一点.
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| 关 键 词： | s-过程核素 r-过程核素 双超丰 贫金属星 |
The Formation of the s-process and r-process Nuclei Double Super-rich Star |
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| LIU Qing-hua. The Formation of the s-process and r-process Nuclei Double Super-rich Star[J]. Journal of Gansu Lianhe University :Natural Sciences, 2011, 25(3): 37-39 |
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| Authors: | LIU Qing-hua |
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| Affiliation: | LIU Qing-hua(Physics Department of Xingtai University,Xingtai 054001,China) |
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| Abstract: | Slow neutron capture and rapid neutron capture process nuclei double super-abundance star is first polluted by AGB star and then formed by the outbreak of the supernova.This can be confirmed by analyzing double super-abundance metal poor star HE 1305-0007. |
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| Keywords: | s-process nuclei r-process nuclei abundance metal-poor stars |
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