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通过超大质量黑洞的反来抑制早期类型星系中的恒星形成
Kevin Schawinski1, Sadegh Khochfar, Sugata Kaviraj
1Department of Physics, University of Oxford, Oxford OX1 3RH, UK.
Nature
|August 25, 2006
概括
超大质量黑洞通过驱逐气体来调节星系进化,抑制大质量星系中的恒星形成. 这种反机制对于理解星系恒星形成历史至关重要.
科学领域:
- 天文学和天体物理学
- 银河系的进化 银河系的进化
- 黑洞物理学 黑洞物理学
背景情况:
- 超大质量黑洞位于银河系中心,并通过反影响宿主星系.
- 在黑洞特性和宿主星系特征之间存在观察到的关系.
研究的目的:
- 为了研究超大质量黑洞反在大质量早期类型星系中的作用.
- 为了获得影响恒星形成的临界黑洞质量的经验关系.
主要方法:
- 高分辨率观测来自大质量早期类型星系的紫外线辐射.
- 分析黑洞质量和宿主星系的速度分散.
主要成果:
- 对一个临界黑洞质量得出了一个经验关系.
- 在这个临界质量以上的黑洞的外流通过加热和驱逐冷气体来抑制恒星形成.
结论:
- 超大质量黑洞,尽管它们的质量很小,但它们对银河系的恒星形成历史产生了重大影响.
- 黑洞反是大质量星系中恒星形成调节的关键机制.
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