Fig. 9
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The eccentricity distribution (left panel) and mass ratio distribution (right panel) of ProCeps and Cepheids in binaries. The solid, dotted and dashed line shows the distribution at t0, tTAMS, and tHe,end, respectively. The plot is for Cepheids formed in a population of star clusters with Rg = 8 kpc, Z = 0.014, and of the adopted ECMF of slope β = 2 Eq. (4).
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