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Fig. 10

image

[X/H] 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 disks. Blue dots represent thin disk stars with [Ti/Fe] < 0.2, while red dots indicate thick disk stars identified with [Ti/Fe] > 0.2. The average error on the abundance ratio is indicated in black.

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