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Fig. 17.

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Mass outflow rate (left), outflow momentum rate (middle), and outflow kinetic luminosity (right) as a function of SFR. Lightblue and orange symbols indicate SB- and AGN-dominated nuclei, respectively. Circles indicate interacting systems and squares indicate mergers from the PUMA sample (including nuclei with log LIR/L < 11.8). Stars show the PHANGS-ALMA targets from Stuber et al. (2021). A representative errorbar is shown on the lower right. Left panel: the black dotted-dashed lines show lines of constant mass-loading factors (η = out/SFR) of 0.1, 1 and 10. Middle panel: the dashed line indicates the total momentum injected by SNe as a function of SFR. The dotted line shows the LSFR/c ratio, where LSFR is the IR luminosity for a given SFR derived using the Kennicutt & Evans (2012) relation. Right panel: the lines show the 1%, 10% and 100% of the energy produced by SNe. The lightblue lines in the three panels are the best linear fit to the data, with the shaded area indicating the 1σ uncertainty.

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