MHD Accretion Disk Winds: The Key to AGN Phenomenology?
Accretion disks are the structures which mediate the conversion of the kinetic energy of plasma accreting onto a compact object (assumed here to be a black hole) into the observed radiation, in the process of removing the plasma’s angular momentum so that it can accrete onto the black hole...
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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/2075-4434/7/1/13 |