A broken neutron-star remnant mass relation plus weak ultra-stripped supernova kicks can reproduce the apparent eccentricity gap in Galactic double neutron stars.
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On Bimodality in the Eccentricity Distribution of Galactic Double Neutron Stars
A broken neutron-star remnant mass relation plus weak ultra-stripped supernova kicks can reproduce the apparent eccentricity gap in Galactic double neutron stars.