在进化的二进制系统中追踪化学物质耗尽,以容纳第二代过渡磁盘
Maksym Mohorian1,2, Devika Kamath1,2,3, Meghna Menon1,2
1School of Mathematical and Physical Sciences, Macquarie University, Balaclava Road, Sydney, NSW 2109, Australia.
概括
与其他恒星相比,在具有过渡盘的双星中,化学耗尽显著更高. 这些AGB后/RGB后的恒星表现出类似于星际介质的枯竭模式,提供了对环双星盘化学的见解.
科学领域:
- 天体物理学 天体物理学
- 恒星进化 恒星进化
- 天体化学是天体化学.
背景情况:
- 在天体物理环境中的化学耗尽机制仍然不太了解.
- 带有过渡盘的后非对称巨分支 (后AGB) 和后红巨分支 (后RGB) 恒星提供了独特的实验室来研究这些过程.
研究的目的:
- 研究具有过渡盘的AGB后/RGB后二进制恒星中的化学耗尽.
- 将耗尽效率和模式与其他恒星群体和星际介质进行比较.
主要方法:
- 使用HERMES/Mercator和UVES/VLT的高分辨率光学光谱学.
- 详细的化学丰度分析 (1D LTE和1D NLTE校正) 对元素C到Eu.
- 分析丰度和二进制系统参数之间的相关性.
主要成果:
- 用[S/Ti]表示的耗尽效率,在具有过渡盘的后AGB/后RGB二进制文件中更高.
- 在这些星系中,耗尽的强度明显高于具有过渡盘的年轻恒星.
- 挥发性和耐火性元素的[X/Zn]丰度比率通常类似于星际介质的趋势.
结论:
- 具有过渡盘的后AGB/后RGB二进制显示增强的化学耗尽.
- 耗尽模式为环双星磁盘内的耗尽机制提供间接约束.
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