Fig. 9
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[X/Fe] as a function of age for stars with an error in age smaller than 1.5 Gyr. We note the different size of y axis for oxygen withrespect to the rest of elements. The red, blue, and black lines are weighted linear fits to thin disk stars with [Fe/H] > 0.2 dex, –0.2 < [Fe/H] < 0.2 dex and –0.6 < [Fe/H] < –0.2 dex, respectively.
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