Magnetic origin of black hole winds across the mass scale

Volume: 1, Issue: 4
Published: Mar 6, 2017
Abstract
Invariably, black hole accretion disks seem to produce plasma outflows that result in blue-shifted absorption features in their spectra1. The X-ray absorption-line properties of these outflows are diverse, ranging in velocity from non-relativistic2 (~300 km s–1) to sub-relativistic3 (~0.1c, where c is the speed of light) and a similarly broad range in the ionization states of the wind plasma2,4. We report here that semi-analytical, self-similar...
Paper Details
Title
Magnetic origin of black hole winds across the mass scale
Published Date
Mar 6, 2017
Volume
1
Issue
4
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