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Fig. 7.

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Final results for NGC 1835 in comparison with other clusters. Left panel: relation between Nrelax and A rh + $ A^+_{\mathrm{rh}} $ for the star clusters homogeneously investigated so far through the dynamical clock approach: the 52 Galactic GCs discussed in Ferraro et al. (2023) are shown as grey circles, the five LMC clusters discussed in Ferraro et al. (2019) are plotted as yellow squares, the two young star clusters in the SMC discussed in Dresbach et al. (2022) are marked as yellow diamonds, and the determination of NGC 1835 obtained in this work is plotted as a filled red square. Right panel: relation between rc and A rh + $ A^+_{\mathrm{rh}} $ for the same star clusters plotted in the left panel (same symbols).

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