Fig. 5.
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Examples of the pixel-by-pixel Tdust − ΣSFR (left panels) and Tdust − ΣM* (right panels) correlations for two sample galaxies (NGC 2403 and NGC 5055). The colour bar represents the galaxy radius. The weighted Pearson correlation coefficient r (top-left corner) and the sampled physical scale (bottom-right corner) are quoted in the panels.
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