Are GRMHD Mean-Field Dynamo Models of Thick Accretion Disks SANE?
The remarkable results by the Event Horizon Telescope collaboration concerning the emission from M87* and, more recently, its polarization properties, require an increasingly accurate modeling of the plasma flows around the accreting black hole. Radiatively inefficient sources such as M87* and Sgr A...
| Hlavní autoři: | , , , |
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| Médium: | Článek |
| Jazyk: | English |
| Vydáno: |
MDPI AG
2021-07-01
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| Edice: | Universe |
| Témata: | |
| On-line přístup: | https://www.mdpi.com/2218-1997/7/8/259 |