Fig. 10
Run of the ratio rCN = nCNstrong/nCNweak for our sample clusters. In each panel, NGC 362 ans Pal 12 (grey dots) are excluded from the relations. Dotted lines mark linear fits to the remaining clusters (black dots) and the correlation coefficients are reported on top of each panel: rS stands for the Spearman and rP for the Pearson coefficient. For the meaning of X labels, see Tables 3 and 4.
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