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Fig. 7


Left: fraction of Mdust heated by radiation fields stronger than that of the diffuse ISM (or equivalently by U > Umin) as a function of the L24/LIR ratio for star-formation-dominated sources with EW6.2 > 0.5  μm (black circles) and 0.2  μm <EW6.2 ≤ 0.5  μm (purple circles). The orange line depicts the best fit to the data. Right: dust mass heated by U > Umin versus . Both quantities are normalised by LIR. The purple lines donate the best fit to the data and a scatter of 0.2 dex.

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