The distributions of key physical paramters for the new sampled clusters. The left subfigure shows the number of stars as a function of the distance to the cluster’s centre of mass for a set of simulated clusters, DMCMC and EMCMC (three clusters each). On the right subfigure is plotted a histogram of the angular momentum distribution of the stars for the same sets of clusters as in the left subfigure. The angular momentum is measured in the units of the international system.