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Fig. 16


Examples of the abundance distributions in the discs of galaxies with available SDSS spectroscopy. The grey points stand for abundances in individual regions (spaxels) obtained from the CALIFA spectra. The dashed (black) line indicates a purely linear fit to those data; the solid (red) line indicates a broken linear fit. The dark (black) points denote the oxygen abundances determined from the SDSS spectra.

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