Notes. Column (1): Total number of Gaussians used for each line, Line and Component considered. Column (2): velocity shear, defined as half of the difference between the median value of the 5 percentile at each end of the velocity distribution: $v_{\mathrm{shear}}=\frac{1}{2}$ (v_max^5% − v_min^5%). Column (3): mean (median) velocity offset between the secondary or tertiary component and the primary component (i.e., Δv = v_i − v_sys, for i = S or T). Column (4): mean (median) velocity dispersion. Column (5): mean (median) velocity dispersion derived within the area covered by the outflow. Column (6): (observed) dynamical ratio, defined as the ratio between the v_shear (Column 2) and σ_mean (Column 4). All these kinematic values include the contribution from the companion galaxy.