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Fig. 7.

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Pearson correlation coefficient r of the Tdust − ΣSFR relation vs that of the Tdust − ΣM* relation. AGN galaxies are marked with stars, non-AGN galaxies with circles. The galaxies are colour-coded according to the p-values of the χ2 test (see Sect. 3.3.2): blue symbols to p < 0.05 (aligned with the young star-driven heating assumption: YS) and orange symbols correspond to p ≥ 0.05 (deviation from the young star heating assumption: not YS). The black dashed line represents the 1:1 relation. The grey histograms in the margins show the distributions of the correlation coefficients for Tdust − ΣSFR (top) and Tdust − ΣM* (right).

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