Ratio of wind velocity and galaxy escape velocity (Table 4) plotted against the dynamical mass (left), and the Hα dynamical ratio from Bellocchi et al. (2013) (right). These plots are color coded by the logarithm of the SFR and disk thickness of the ionized gas disks (Table 4), respectively, right and left. The green horizontal line indicates where V_w/v_esc is 1. In the right panel, galaxies with no dynamical mass estimation (F05189-2524 and F07027-6011 (N); Bellocchi et al. 2013) are indicated with circles (as Fig. 10).