Abundance to age ratios in the HARPS-GTO sample with Gaia DR2 - Chemical clocks for a range of [Fe/H]

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Fig. 10

Slopes (dex Gyr⁻¹) of the [X/Fe]-age relations ([X/Fe] = a + b⋅Age) for neutron capture elements as a function of s-process contribution for thin disk stars att all metallicities and in four metallicity bins with a width of 0.4 dex.

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