Fig. 13
Left panel: SPIRE colour F250/F350 against star formation rate surface density. Symbols are the same used in Fig. 12. The dotted line is a least square fit to the DGS and KINGFISH dwarf galaxies. Right panel: SPIRE colour F250/F350 against stellar mass surface density Pearson correlation coefficients for the different samples are displayed at the top-left corner of each panel. The mean error bars are displayed at the bottom-right corner of each panel.
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