Hot Accretion Flow in Two-Dimensional Spherical Coordinates: Considering Pressure Anisotropy and Magnetic Field
For systems with extremely low accretion rate, such as Galactic Center Sgr A* and M87 galaxy, the ion collisional mean free path can be considerably larger than its Larmor radius. In this case, the gas pressure is anisotropic to magnetic field lines. In this paper, we pay attention to how the proper...
Furkejuvvon:
| Váldodahkkit: | , |
|---|---|
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
MDPI AG
2019-09-01
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| Ráidu: | Universe |
| Fáttát: | |
| Liŋkkat: | https://www.mdpi.com/2218-1997/5/9/197 |
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