Structural parameters, chronological age, and dynamical age of the Large Magellanic Cloud globular cluster NGC 1754

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Fig. 9

Relation between N_relax and $A_{r h}^{+}$ $A_{r h}^{+}$ (left) and between r_c and $A_{r h}^{+}$ $A_{r h}^{+}$ (right) for star clusters analyzed using the dynamical clock method. NGC 1754 is represented by a large red square, and the 52 Galactic GCs discussed in Ferraro et al. (2023) by gray circles. The six old LMC clusters from Ferraro et al. (2019) and Giusti et al. (2024b) are plotted as yellow squares, and the two young Small Magellanic Cloud clusters from Dresbach et al. (2022) as yellow diamonds.

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