A super-Eddington accretion model with population synthesis attributes the 1.8 Msun NS mass peak to short-period low-mass donor systems and the 1.4 Msun peak to common-envelope evolution.
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Mass distribution of neutron stars in binary systems
A super-Eddington accretion model with population synthesis attributes the 1.8 Msun NS mass peak to short-period low-mass donor systems and the 1.4 Msun peak to common-envelope evolution.