早期宇宙中低质量星系的反
1Center for Gravitation, Cosmology and Astrophysics, Department of Physics, University of Wisconsin Milwaukee, 3135 North Maryland Avenue, Milwaukee, Wisconsin 53211, USA.
Nature
|July 10, 2015
概括
巨大的恒星反驱动银河系的外流,并调节恒星形成. 这一过程也使电离辐射逃逸,使早期宇宙重新电离.
科学领域:
- 天体物理学 天体物理学
- 宇宙学的宇宙学是什么?
- 银河系的进化 银河系的进化
背景情况:
- 巨大的恒星释放出大量的能量和动量,这个过程被称为恒星反.
- 恒星反在通过加热或驱逐星际气体来调节恒星形成方面发挥着至关重要的作用.
- 由反驱动的银河系外流被观察到,特别是在恒星形成的星系和早期宇宙中.
研究的目的:
- 为了研究恒星反在银河系进化中的作用.
- 了解反如何影响恒星形成率.
- 探索反对宇宙再电离的贡献.
主要方法:
- 观测天文学研究银河系规模的外流.
- 分析恒星形成区域中的气体特性.
- 宇宙模拟用于模拟早期宇宙过程.
主要成果:
- 恒星反被证实通过气体去除和加热来抑制恒星形成.
- 星系外流是高恒星形成率星系中常见的现象.
- 低质量星系的反可能促进了电离辐射的逃逸.
结论:
- 恒星反是调节星系生长和恒星形成的关键机制.
- 早期宇宙中的反过程对于宇宙再电离是至关重要的.
- 了解反对于理解星系进化和星系间介质至关重要.
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