Magnetic confinement of broad-line clouds in active galactic nuclei
Magnetic confinement of broad-line clouds in active galactic nuclei
复制标题
活动星系核中宽线云的磁约束
DOI：
10.1093/mnras/228.1.47p
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发表时间：
1987
影响因子：
4.8
通讯作者：
M. Rees
中科院分区：
文献类型：
--
作者：
M. Rees
包含在活动星系核中发射宽谱线的云的区域可能被强度约为 1 G 的磁场所遍布。磁应力可以限制云，从而消除了与云压力平衡的康普顿加热介质的需要。
The region containing the clouds that emit the broad spectral lines in active galactic nuclei may be pervaded by a magnetic field of strength ∼1 G. Magnetic stresses could then confine the clouds, obviating the need for a Compton-heated medium in pressure balance with the clouds.