Fig. 14
Same as Fig. 13, but for a system where a BH would be expected to form from the secondary. We assume that 10% of the stellar mass is lost during BH formation, and that the BH receives a kick with a 1D rms of σ = 26.5kms-1. Kick velocities up to v = 135 km s-1 are considered in the top panel, which corresponds to 99.999% of the Maxwellian distribution.
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