Physics of “Cold” Disk Accretion onto Black Holes Driven by Magnetized Winds
Disk accretion onto black holes is accompanied by collimated outflows (jets). In active galactic nuclei (AGN), the kinetic energy flux of the jet (jet power or kinetic luminosity) may exceed the bolometric luminosity of the disk by a few orders of magnitude. This may be explained in the framework of...
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| Format: | Article |
| Language: | English |
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MDPI AG
2019-01-01
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| Series: | Galaxies |
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| Online Access: | http://www.mdpi.com/2075-4434/7/1/18 |