Fig. 13.
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parameter as a function of dynamical age Nh. The black circles are the GCs analysed in Dalessandro et al. (2019a; see also Smolinski et al. 2020), and the red square is NGC 2419. The blue and green lines show the results of the N-body simulations presented by Dalessandro et al. (2019a) following the 
evolution of clusters born with a FP half-mass radius of five and ten times larger than that of SP stars, respectively.
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