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Fig. 14


Distribution of the scatter relative to the radial abundance gradients as a function of: presence of bars (A, clearly unbarred galaxies; B, clearly barred; AB, intermediate stage; top left), environment of the galaxy (S, isolated; G, in group; P, paired, I, in interaction; top middle), numerical morphological type according to the de Vaucouleurs system (T, top right), specific star formation rate (bottom left), integrated stellar mass (bottom middle), and stellar mass density at one disc effective radius (bottom right). The black squares represent the mean values within each segregation, with the errorbars indicating the standard deviation. See text for details of the derivation of these parameters.

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