Numerical simulations of the line-force-driven winds from active galactic nuclei: The special relativistic effects

Open Access

Fig. 6.

Angular profiles of time-averaged variables. Panel (A): the angular profiles of the column density; Panel (B): the angular profiles of the density at r = 1500r_s; Panel (C): the angular profiles of the radial velocity at r = 1500r_s; Panel (D): the angular profiles of the mass flux density at r = 1500r_s. In panel (A), the horizontal line means the column density of 10²² cm⁻². In panel (C), the horizontal line means the velocity of 10⁴ km s⁻¹.

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