https://www.mdpi.com/2218-1997/5/4/89
Self-Similar Solution of Hot Accretion Flow with Anisotropic Pressure
For the accretion flow in extremely low-luminosity active galactic nuclei, such as our Galactic center (Sgr A*) and M 87, the collisional mean-free path of...
self similar solutionhotaccretionflowanisotropic