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Fig. 1

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Left panel: evolution of Rh for nTD-MSP model (dash-dotted black line), and TD-MSP model (solid black line), and evolution of the total cluster mass for nTD-MSP model (solid red line), and TD-MSP model (solid red line). Right panel: evolution of the ratio N2/Ntot for the nTD-MSP model (dash-dotted black line), and TD-MSP model (solid black line). The global cluster parameters are listed at the top of each panel: N1− number of 1P objects, N2 – number of 2P objects, Z – metallicity, Rg – galactocentric distance (size of the circular orbit), TF – tidally filling 1P, Wo1− King parameter for 1P, conc – concentration parameter (concpop = Rh 2/Rh1), bf – binary fraction, Q1− virial ratio for 1P. Unless otherwise noted, all figures from now on are made for the parameters tstart = 0.5 * tdelay and tend = tdelay = 100 Myr.

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