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Fig. 10

image

Wind loading factor plotted against the infrared luminosity (left, Table 1) and dynamical mass (right) color coded by the logarithm of the SFR. In both panels, those galaxies for which we were unable to infer the wind morphology in detail are indicated with an additional square. In the left panel, the galaxies that lack of a reliable estimation of the dynamical mass (F05189-2524 and F07027-6011 (N); Bellocchi et al. 2013) are shown with circles.

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