Free Access

Fig. 10


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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.