Fig. 8
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(a and b) Histograms of ASCC 71 and ESO 064-05 orbital separations at 56 Myr ago and at 100 Myr in the future. (c and d) Histograms of NGC 2129 and UBC 437 orbital separations at 46 Myr ago and at 100 Myr in the future. The solid line represents the orbital separation calculated using the cluster mean property parameter. The dashed line represents the mean value of the orbital separation obtained using the MC sampling over the measured uncertainties in cluster property parameter.
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