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...
Αποθηκεύτηκε σε:
| Κύριοι συγγραφείς: | , , , |
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| Μορφή: | Artigo |
| Γλώσσα: | Inglês |
| Έκδοση: |
MDPI AG
2021-07-01
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| Σειρά: | Universe |
| Θέματα: | |
| Διαθέσιμο Online: | https://www.mdpi.com/2218-1997/7/8/259 |
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