Fig. 10.
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[Y/Mg] abundances of the sample of clusters from Casamiquela et al. (2021) in grey, and the linear fit computed. The values of the Hyades, NGC 2632 and Ruprecht 147 clusters are highlighted. The value computed in this paper for UBC 274 is plotted as a red square. Top plot: shows the clusters closer than d < 1 kpc, and the bottom plot shows all the clusters in the sample.
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