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Fig. 11

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Correlation between the warm dust luminosity and the combination of Hα and 24 μm IR luminosities for NGC 1313 (open circles), M81 (filled circles) and M101 (open crosses). The dashed line shows the best-fit linear model with a unity slope for all data points for NGC 1313, M101, and M81. The data plots for M101 and M81 are taken from Suzuki et al. (2010). The scaling factor for the 24-μm IR luminosity is taken from Calzetti et al. (2010).

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