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Fig. 9
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Dependence of [X/Fe] on galactocentric radius. OCCASO+ data (Carbajo-Hijarrubia et al. 2024) are represented by triangles. Auner 1 and Berkeley 102 are shown as squares. All the objects are colour-coded by age. The black lines show the MCMC best fits to the OCCASO+ sample as derived by Carbajo-Hijarrubia et al. (2024).
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