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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 9.

Radial profiles of the radial velocity, Mach number, temperature, and density profiles at several different θ angles in the 2D simulation. Colors denote angles of 5° (black), 10° (blue), 20° (dark green), and 30° (light green). The analytic solution of model “hot_bhg_ta” is shown by dashed curves.

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