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Fig. C.2


Distribution of slopes depending on different galaxy properties using the M13-N2 (top panels) and the D16 (bottom panels) calibrators: (i) the environment of the galaxies (isolated, green; in groups, blue; paired, red; interacting, yellow) for the left panel, (ii) the presence or absence of bars (clearly unbarred galaxies, green; clearly barred, red; and an intermediate stage, blue) for the middle panel, and (iii) the shape of the abundance profile (single profile, green; broken profile with inner drop, blue; broken profile with outer flattening, red; and a doubly-broken profile with presence of both inner drop and outer flattening, yellow) for the right panel. The black diamonds represent the mean values within each segregation, with the error bars indicating the standard deviation.

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