Radial profiles of the molecular gas derived with 3DB. From top to bottom: the CO(3 − 2) surface density, the rotational velocity (same as the yellow dots in the top panel of Fig. 6), the velocity dispersion and the outflow velocity, all as a function of deprojected distance from the AGN (on the plane of the galaxy). The dashed black line in the bottom panel is the zero line, dividing between ouflow ($v_{\mathrm{out}}^{\mathrm{mol}}>0$) and inflow ($v_{\mathrm{out}}^{\mathrm{mol}}<0$).