New 3D kinematic reconstruction from SITELLE data resolves a cavity at the base of the Crab Nebula's northern jet and connects it to the filamentary network, implicating the early pulsar wind nebula in jet formation.
H., Kirsten F., Pen U.-L., Deller A
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astro-ph.HE 2years
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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.
citing papers explorer
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3D Kinematic Reconstruction of the Crab Nebula That Includes the Northern Ejecta `Jet'
New 3D kinematic reconstruction from SITELLE data resolves a cavity at the base of the Crab Nebula's northern jet and connects it to the filamentary network, implicating the early pulsar wind nebula in jet formation.
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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.