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Fig. 17.

image

Elemental-to-iron abundance ratios as a function of the mean galactocentric distances. The blue dots and red triangles represent the thin- and thick-disc stars of our study, respectively. The blue lines are the linear fits for the thin-disc stars and the red lines show the thick-disc stars. The uncertainties in [El/Fe] and Rmean were taken into account while computing the slopes. The 95% confidence intervals for the slopes are shadowed. The dotted lines correspond to the solar mean galactocentric distance.

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