一个气体云正在朝着银河系中心的超大质量黑洞前进
S Gillessen1, R Genzel, T K Fritz
1Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany. ste@mpe.mpg.de
Nature
|December 16, 2011
概括
一个密集的气体云正在落入射手座A*,一个超大质量黑洞. 它的轨迹和破坏将揭示黑洞养和积累过程的洞察力.
科学领域:
- 天体物理学 天体物理学
- 天文学 天文学
背景情况:
- 射手座A* (Sgr A*) 是银河系中心的一个超大质量黑洞,大约是太阳质量的400万倍.
- Sgr A* 呈现较低的增积率和辐射效率,除偶尔的X射线和红外发光外,其亮度较弱.
研究的目的:
- 报告发现和轨道特征的密集的气体云接近Sgr A*.
- 为了研究这种气体云与黑洞积聚区相互作用的动态演变和辐射.
- 利用云的相互作用来探测积累流特性和超大质量黑洞养机制.
主要方法:
- 恒星轨道测量证实Sgr A*是一个黑洞.
- 观测天文学用于检测和跟踪气体云的轨迹.
- 对潮剪切和重力作用于气体云的分析.
主要成果:
- 一个密集的气体云,大约是地球质量的三倍,正朝着Sgr A*处于极其古怪的轨道上.
- 云对事件视界最接近的距离大约是视界半径的3100倍,预计在2013年.
- 在过去的三年里,由于Sgr A*引力的潮力,云开始被破坏.
结论:
- 气体云的轨道动态和随后的破坏将为Sgr A*附近的积累过程提供关键数据.
- 未来对云的演变进行观测,可能会发现Sgr A*的X射线辐射显著亮化.
- 云的破裂可能会引发一个主要的辐射耀斑,如果碎片养中央积聚区.
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