Surface critical velocity fraction v/v_crit of our LMC models with different magnitudes as a function of cluster age. Each panel shows the result for the stellar models with a given magnitude, indicated in the legend. M_TO denotes the absolute F814W magnitude of the cluster turnoff. In each panel, different colors correspond to the stellar models with different initial rotational velocities. We show the turn-off mass of the clusters with corresponding ages on the top x-axis in the first panel.