低质量恒星中重元素合成的温度和时间表
P Neyskens1, S Van Eck1, A Jorissen1
1Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles (ULB), CP 226, 1050 Bruxelles, Belgium.
Nature
|January 9, 2015
概括
该研究确定了进化恒星的缓慢中子捕获过程 (s-过程) 温度,支持碳-13作为主要中子源. 这一发现还为恒星中的重元素合成提供了一个时间表.
科学领域:
- 核天体物理学 核天体物理学
- 恒星进化 恒星进化
- 太空化学 太空化学
背景情况:
- 重元素在恒星中通过中子捕获 (s过程) 合成.
- 两个中子源,碳-13和-22,被建议用于s过程.
- 以前的模型偏爱碳-13,但石数据表明虹-22.
研究的目的:
- 直接确定进化低质量巨星中的s过程温度.
- 为了确定负责重元素合成的主导中子源.
- 为了建立一个时间表的s-过程核合成.
主要方法:
- 在演化后的低质量巨星中分析和的丰度.
- 使用放射性双-93/-93和技术-99/-99作为计时器.
- 在不依赖恒星进化模型的情况下,独立确定s过程温度.
主要成果:
- 衍生出的s-过程温度直接支持碳-13作为中子源.
- 该研究为s过程的开始提供了100万到300万年的时间表.
- 调和恒星进化模型和石同位素比率之间的差异.
结论:
- 碳-13被证实是低质量恒星中s过程的主要中子源.
- 这些发现为重元素核合成和恒星化学丰富提供了关键的见解.
- 建立的时间尺度有助于理解银河系化学进化的历史.
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