磁盘积聚到黑洞上的磁性性质
Jon M Miller1, John Raymond, Andy Fabian
1Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, Michigan 48109, USA. jonmm@umich.edu
Nature
|June 23, 2006
概括
黑洞周围的积聚盘是由磁性过程驱动的. 这项研究提供了第一个观察证据,证明磁粘度和磁离心力驱动磁盘积累,证明其基本上是磁性.
科学领域:
- 高能天体物理学 高能天体物理学
- 紧的对象研究研究.
- 黑洞积聚物理 黑洞积聚物理
背景情况:
- 在高能天体物理学中,对紧物体的盘积累至关重要.
- 积累盘中的角运动量转移机制尚不清楚.
- 缺乏关于内部粘度或磁盘风的观测证据.
研究的目的:
- 为了确定驱动磁盘在紧物体上的增积的机制.
- 提供关于积累盘中的角动量转移的观测证据.
- 为了研究磁力过程在黑洞积累中的作用.
主要方法:
- 观测恒星质量黑洞二进制GRO J1655-40的情况.
- 对吸收X射线的风进行了详细的光谱分析.
- 风能发电机制的建模.
主要成果:
- 在GRO J1655-40中发现了一个吸收X射线的风.
- 风是由磁性过程驱动的,特别是磁性粘度或磁离心力.
- 这种磁性过程也驱动了通过磁盘的积累.
结论:
- 黑洞上的磁盘积累基本上是一种磁性过程.
- 磁粘度和磁离心力是角度运动量转移的关键机制.
- 这项研究提供了磁力过程驱动积累的第一个观测证据.
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