发现了三颗富含的恒星
S Van Eck1, S Goriely, A Jorissen
1Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Boulevard du Triomphe, C.P. 226, B-1050 Bruxelles, Belgium. svaneck@astro.ulb.ac.be
Nature
|August 24, 2001
概括
研究人员在三个金属贫困恒星中发现了大量的. 这一发现支持了这样一个理论,即恒星在他们的非对称巨分支阶段通过缓慢的中子捕获过程 (s过程) 合成重元素.
科学领域:
- 天文学 天文学
- 恒星进化 恒星进化
- 核天体物理学 核天体物理学
背景情况:
- 一半比铁重的稳定核在低至中等质量恒星 (0.8-8太阳质量) 中合成.
- 这些元素在非对称巨分支 (AGB) 阶段通过恒星风被驱逐到星际介质中.
- 缓慢的中子捕获过程 (s过程) 从恒星内的铁核中构建出更重的元素.
研究的目的:
- 为了研究金属贫困恒星中和其他重元素的丰富性.
- 测试在非对称巨分支 (AGB) 恒星中核合成模型.
- 为了确认在恒星内部的s过程的运行.
主要方法:
- 在三个贫金属恒星 (HD187861,HD196944,HD224959) 中对元素丰度的分析.
- 用光谱分析来确定恒星的组成.
- 观测到的丰度与来自恒星核合成模型的预测进行比较.
主要成果:
- 在三个研究的贫金属恒星中发现了大量的丰富.
- 观测到的丰度在这些恒星中高于其他重元素.
- 和其他重元素的观察和预测丰度之间有很好的一致性.
结论:
- 这些发现支持了通过AGB恒星中的s过程合成重元素的理论.
- 这项研究加强了对低金属度恒星环境中的核合成的理解.
- 观察到的过剩与早期银河系AGB恒星中运行的s过程模型相一致.
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