Fig. 3

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Relationship between [Ce/Fe] and [Fe/H], age, and Rgc (left) and [Ce/H] as a function of [Fe/H], age, and Rgc (right). Data for field stars taken from Ryde et al. (2020) are shown as gray dots. The clusters taken from Myers et al. (2022) are shown as light gray squares. The slopes 0.049 ± 0.03 and −0.068 ± 0.047 (shown in the figure) were obtained by incorporating the calculations of NGC 6791 into the plot.
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