在积聚超大质量黑洞附近的动态重要磁场
M Zamaninasab1, E Clausen-Brown1, T Savolainen1
1Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.
Nature
|June 6, 2014
概括
超大质量黑洞发射喷射器具有动态重要磁场. 这些场与积累盘的亮度相关,影响喷气形成和黑洞积累过程.
科学领域:
- 天体物理学 天体物理学
- 黑洞物理学 黑洞物理学
- 等离子体物理学的物理学
背景情况:
- 积聚的超大质量黑洞会产生相对论喷射.
- 假设磁场对喷气形成和积累盘物理至关重要.
- 以前的观测表明,银河系中心黑洞附近具有动态重要磁场.
研究的目的:
- 研究喷射发射区域中的磁场与积累盘亮度之间的关系.
- 为了确定是否动态重要磁场在无线电响亮的活跃星系中很常见.
- 了解这些磁场对积累盘属性和喷气动力学的影响.
主要方法:
- 分析了76个无线电响亮活跃星系的样本.
- 喷射磁场强度与增积盘亮度在七个数量级上的相关测量.
主要成果:
- 在喷气式磁场强度和积累盘亮度之间发现了密切的相关性.
- 这种相关性跨越了七个数量级,表明有一个普遍的关系.
- 在这些星系的喷射发射区域中存在动态重要磁场.
结论:
- 无线电高频活跃星系的喷射发射区域由动态重要磁场线.
- 这些磁场显著影响了积累盘的特性,包括气体的入射和角运动量传输.
- 磁场在决定喷气的方向性和形成方面发挥着至关重要的作用.
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