Top left: distribution of H II region escape velocities in galaxy centers and disks. Middle left: distribution of pressures due to H II region self-gravity for ﹩{M}_{{\rm{sh}}}=50 \% {M}_{{\rm{Mol}}}^{{\rm{init}}}﹩ (fiducial value; solid gray), ﹩60 \% {M}_{{\rm{Mol}}}^{{\rm{init}}}﹩ (dashed gray), and ﹩70 \% {M}_{{\rm{Mol}}}^{{\rm{init}}}﹩ (dotted–dashed gray); disk 〈P_DE〉 (from J. Sun et al. 2023; maroon); fiducial P_Grav + 〈P_DE〉 (purple), and total P_Feedback (green). Bottom left: distribution of H II region R_circ (gray hatches) and the sizes at which we expect P_Grav = 〈P_DE〉 (maroon), P_Grav = P_Feedback (green), and P_Grav + 〈P_DE〉 = P_Feedback (purple). Right: H II region overpressure (shaded blue) vs. underpressure (shaded orange) for P_Feedback/P_Grav (gray) and P_Feedback/(P_Grav + 〈P_DE〉) (purple; the dashed line indicates the median, with a summary histogram to the right) with 5th/16th/25th/50th/75th/84th/95th percentile contours.