Kinematic distances for 66 pulsars are computed from archival HI radial velocities using a modern Galactic rotation curve and show agreement with independent parallax measurements within 1 sigma for nearly all objects with both.
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Characterizing Pulsar Distances Using HI Kinematics
Kinematic distances for 66 pulsars are computed from archival HI radial velocities using a modern Galactic rotation curve and show agreement with independent parallax measurements within 1 sigma for nearly all objects with both.