A relation between the radial velocity dispersion of young clusters and their age - Evidence for hardening as the formation scenario of massive close binaries

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Fig. 4.

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P_cutoff versus age of the clusters. The error bars represent the P_cutoff corresponding to the distributions that represent each σ_1D within their 68% confidence range. The blue line and shaded region show the fit to the data and its 1-σ error bars.

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