巨型黑洞的近距离环境是由辐射反形成的
Claudio Ricci1,2,3, Benny Trakhtenbrot4, Michael J Koss4,5
1Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile.
Nature
|September 30, 2017
概括
超大质量黑洞的辐射反会调节气体和尘埃的遮蔽. 这种由质量正常化的积累率驱动的反会在黑洞的帕塞克内清除环核物质.
科学领域:
- 天文学与天体物理学
- 宇宙尘埃和气体动力学
- 超大质量黑洞积聚
背景情况:
- 大多数超大质量黑洞都被气体和尘埃所遮蔽.
- 这种模糊材料的分布和演变仍在争论中.
- 随着增积率的增加,观察到遮蔽材料的减少.
研究的目的:
- 确定控制超大质量黑洞周围变暗的主要物理机制.
- 为了澄清环核物质在黑洞积聚中的作用.
- 了解暗黑洞与未暗黑黑洞之间的区别.
主要方法:
- 对硬X射线黑洞进行了系统的多波长调查.
- 分析的气体柱密度,亮度和质量数据.
- 研究了积累率与环核物质分布之间的关系.
主要成果:
- 尘埃状气体的辐射反是控制环核物质的主要机制.
- 在黑洞的几十个帕塞克之内,
- 即使在较低的辐射输出速度下,环核物质也可以分散.
结论:
- 质量正常化的积累率是区分暗黑洞和无暗黑洞的关键驱动因素.
- 辐射反在清除遮蔽物质方面起着至关重要的作用.
- 了解环核物质分布对于黑洞积累研究至关重要.
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