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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 1.

Physical quantities of winds as a function of θ at r = 103rg from the 3D GRMHD simulation of black hole accretion in Y15. Top panels: density, temperature, and Mach number. Bottom panels: radial, meridional, and rotational velocities normalized by Keplerian velocity ﹩{v}_{k}({r}_{0})﹩. The value of the density is shown in code units. The density and temperature are time-averaged values, while all three velocity components are taken from one snapshot.