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Fig. 7


[X/Fe] for neutron-capture elements compared to age. Only stars with age uncertainties less than 3 Gyr are plotted. The vertical dotted line at 8 Gyr indicates an approximate age separation between thin and thick disk. Blue dots represent young thin disk stars, while red dots are for old thick disk stars. The blue and red lines indicate the best fit for thin and thick disk stars. The errors on the ages are from Bensby et al. (2014). The average error on the abundance ratio is indicated in black.

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