Large-scale Dynamics of Winds Originating from Black Hole Accretion Flows. I. Hydrodynamics
Authors: Can Cui, Feng Yuan, and Bo Li
2020 The Astrophysical Journal89080.
Provider: AAS Journals
Caption: Figure 6.
Radial profiles of the radial velocity, Mach number, temperature, and density of the transonic solutions“ hot_bhg_ta,” “hot_bhg_tb” and the supersonic solution “hot_bh_sup,” with detailed boundary parameters as listed in Table 1.