Mass-outflow rates (lower panel) and outflow velocity (upper panel) as a function of distance. Colors show different runs, and line styles different halo mass bins. In all mass bins, the outflow rate and velocities are suppressed throughout the halo in TNG-CR with respect to the fiducial TNG case. In the Milky Way-mass range, the outflow rate is suppressed further in TNG-CR-NF, and the radial trend reverses, leading to larger velocities and outflow rates in the outer versus inner halo (≳0.5 R_200c). TNG-Weak CR is typically intermediate between TNG and TNG-CR. We note, however, that the stellar masses are different in the CR runs as compared to fiducial TNG (see main text).