恒星爆发后星系外流的隐藏质量和庞大的空间范围
Todd M Tripp1, Joseph D Meiring, J Xavier Prochaska
1Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA. tripp@astro.umass.edu
概括
银河系风对于银河系进化至关重要. 这项研究揭示了银河系外流中的热热等离子体含有比以前认为的质量要多得多,这影响了银河系的积聚.
科学领域:
- 天体物理学 天体物理学
- 银河系的进化 银河系的进化
- 等离子体物理学的物理学
背景情况:
- 理论上,多相等离子体外流可以调节星系的生长.
- 对这些流出,特别是热热阶段的观测约束仍然有限.
研究的目的:
- 为了研究恒星爆发后星系风中的温暖热等离子体的质量和范围.
- 了解银河系外流中不同等离子体相之间的关系.
主要方法:
- 利用紫外线吸收光谱来探测温热等离子体相.
- 分析冷和热热气体组件的动力学.
主要成果:
- 在恒星爆发后的星系风中,热热的等离子体 (10^5.5 K) 的质量是冷气体的10-150倍.
- 外流延伸到超过68千帕塞克,其中很大一部分可能逃离银河系.
- 动力学相关性表明,冷气体与更热,未见的等离子相 (>10^6 K) 之间存在相互作用.
结论:
- 多相风在从星系中移除大量质量的过程中起着至关重要的作用.
- 这些风极大地影响了星系爆发后星系的进化路径.
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