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Updated: Jul 11, 2025

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超大质量黑洞的养和反观察到的小部分尺度
Takuma Izumi1,2,3, Keiichi Wada4,5,6, Masatoshi Imanishi1,3
1National Astronomical Observatory of Japan, Tokyo 181-8588, Japan.
概括
活跃的星系养超大质量黑洞, 但大部分气体是通过外流而不是积聚而排出的. 这项研究揭示了密集,不稳定的气体盘如何在圆环星系的核中驱动积聚.
科学领域:
- 天体物理学
- 银河系的演变
- 黑洞积聚
背景情况:
- 活跃的星系有超大质量黑洞 (SMBH),它们通过增加周围的星系物质而生长.
- 在活跃星系的中央10个帕塞克内直接观察积聚过程是具有挑战性的,因为它们的角大小很小.
研究的目的:
- 在Circinus星系的活跃核中研究子粒子尺度上的积聚过程和气体动力学.
- 在附近的活跃星系核中解决以前未被观察到的积聚机制.
主要方法:
- 使用亚毫米干扰测量来观察圆环星系的活跃核.
- 分析的重点是解决气体的进出量.
主要成果:
- 在Circinus星系中检测到密集的分子气体.
- 只有不到3%的进气被SMBH积累;其余的气体通过多相流出.
- 一个围绕着流入的重力不稳定的,密集的气体盘被确定,在中央帕塞克内驱动积累.
结论:
- 大多数活跃的银河系核中的气体流量都被射出,在银河系反中起着至关重要的作用.
- 在密集的气体盘中引力不稳定是推动SMBH积聚的关键机制.
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