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...
| 出版年: | Universe |
|---|---|
| 主要な著者: | , , , |
| フォーマット: | 論文 |
| 言語: | 英語 |
| 出版事項: |
MDPI AG
2021-07-01
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| 主題: | |
| オンライン･アクセス: | https://www.mdpi.com/2218-1997/7/8/259 |