View of the kinematic model of the molecular torus described in Sect. 7 projected along the line of sight. The arrows represent the velocity field of the gas in the torus (with Keplerian rotation) and over the working surface of the AGN wind on the torus (with outflowing motions). The arrows are color-coded using red, yellow, and blue according to the absolute value and the sign of the radial velocities projected along the line-of-sight measured relative to v_sys. The major axis of the modeled torus has the orientation of the observed torus (PA ≃ 113°). The adopted inclination (i ≃ −70°) is lower than the average value found by ^3DBarolo (i ≃ −80°) for a better illustration of the different velocity components of the model.