Fig. 10.
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Dispersion in Auriga galaxies’ MIR-FIR color-color plot as a function of the non-parametric indicators of galaxy morphology applied to the SFRD maps. The data includes all the three inclinations and all Auriga galaxies except AU-11, which is undergoing a merger. The data-points are color-coded using the Pearson correlation coefficient obtained for the color-color relation for individual galaxies.
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