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This article has an erratum: [https://doi.org/10.1051/0004-6361/201628601e]


Fig. 9

image

Histograms and relations of the properties derived from the linear fittings through the radial scale both for O/H and N/O in those galaxy discs of the CALIFA sample with enough star-forming H ii regions. From top to bottom: correlation coefficient, slope of the gradient, and predicted value at the effective radius of the galaxy.

This figure is made of several images, please see below:

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