Fig. C.1.
Relation between sSFR and fyoung, shown for the radiation transfer models of: NGC 1365, M 83, M 95, M 100 (this work); M 81 (Verstocken et al. 2020); and M 77 (Viaene et al. 2020). Each galaxy dataset is assigned with a different colour indicated in the lower right corner of the first panel. The solid black line shows the fit from Eq. (4) through the bulk of data cells of every galaxy. Each coloured line shows the best-fitting power-law through the bulk of data cells of every galaxy.
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