Fig. 7.
Initial orbital separation of 105 binaries sampled from the extended Sana et al. (2012) distribution, cf. Eq. (A.1), in blue, and from a log-uniform distribution, in orange. Both distributions sample the range p ∈ [0.4, 105.5] days and are independent of metallicity. With a solid line, we show the same distributions after removing systems with Roche-lobe overflow at ZAMS for Z = 0.1 Z⊙.
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