Middle-aged PWNe exhibit diverse reverberation-phase evolution but converge to Sedov-like states; 2D instabilities increase apparent size by up to 50% without changing global dynamics, supporting 1D model robustness.
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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.
citing papers explorer
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Modelling the Dynamics of Middle-Aged Pulsar Wind Nebulae in the Reverberation Phase
Middle-aged PWNe exhibit diverse reverberation-phase evolution but converge to Sedov-like states; 2D instabilities increase apparent size by up to 50% without changing global dynamics, supporting 1D model robustness.
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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.