PSR J1921+3745 lies in the tidal tail of NGC 6791, indicating long-term retention followed by tidal stripping as a source of Galactic neutron stars consistent with low-kick electron-capture supernova formation.
ANewElectron-densityModelfor Estimation of Pulsar and FRB Distances
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A pulsar escaping an ancient open cluster via tidal stripping
PSR J1921+3745 lies in the tidal tail of NGC 6791, indicating long-term retention followed by tidal stripping as a source of Galactic neutron stars consistent with low-kick electron-capture supernova formation.