Relative contribution of the cold molecular (turquoise), ionized (pink), and warm molecular (blue) phases to the total mass outflow rate. The blue labels refer to the relative contribution of the warm molecular phase in %. The galaxies whose names are in violet are the targets of this work. The ionized mass outflow rates are from SP24, adopting their [S II]-based electron densities and divided by us by a factor of 3 to match our outflow geometry. The cold molecular mass outflow rates are from Scenario II in Audibert et al. (2024), and the warm molecular mass outflow rate of J1509 is from Ramos Almeida et al. (2019). No warm molecular outfflow detections are yet reported for J1100.