Fig. C.1
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Histograms of the relative frequency distribution of the main orbital parameters of surviving binaries. The dashed lines indicate the analytical prediction of surviving binaries based on simple criteria (Eqs. (C.7) and (C.9)), while the solid lines depict the results from the three-body numerical simulations (Fig. 2). We show the orbital period (a), eccentricity (b), mutual inclination (c), and mass ratio (d).
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