Figure 6 from Large-scale Dynamics of Winds Originating from Black Hole Accretion Flows. I. Hydrodynamics

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Large-scale Dynamics of Winds Originating from Black Hole Accretion Flows. I. Hydrodynamics

Authors: Can Cui, Feng Yuan, and Bo Li

2020 The Astrophysical Journal 890 80.

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.

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