Fig. 4

Left panels: histograms of the distance in the (r − i) color of the PMS stars from the mean ridge line of the bluest population, as obtained with our Monte Carlo simulations (black, heavy lines) and as observed (red). Right panels: corresponding assumed distribution of the mass ratios of all the binaries in our simulated sample. The χ2 of each solution is also indicated in the left panels. Both top panels correspond to the canonical cases of 40% multiplicity and a uniform mass ratio distribution.
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