Figure 4 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 4.

Radial profiles of radial velocity, Mach number, temperature, and density of the subsonic solution “hot_bh_s” (dashed) and transonic solution “hot_bh_t” (solid) of a wind launched at ﹩{r}_{0}={10}^{3}{r}_{s}﹩, with the detailed boundary parameters listed in Table 1.

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