Fig. 6.
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Expected fraction of eMSPs (black curve, left y-axis) and iMSPs (red and blue curves, right y-axis) as a function of kick velocity, assuming a mass defect of ΔM = 0.016 M⊙. For iMSPs, we consider the systems with eccentricities greater than unity. M2 cannot create eccentric systems due to the rapid re-circularization of the orbit.
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