JWST data reconstructs the inner ejecta of SNR 0540-69.3 as two similar-sized fragmented lobes, implying a ~300 km/s pulsar kick under symmetry assumption and confirming low-velocity hydrogen mixing in a Type II explosion.
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3 Pith papers cite this work, alongside 1 external citations. Polarity classification is still indexing.
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A southern circum-jet ring in the Crab Nebula is identified and attributed to a counterjet within the jittering-jets explosion mechanism framework.
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Exploring the central region of SNR 0540-69.3 with JWST I: 3D morphology
JWST data reconstructs the inner ejecta of SNR 0540-69.3 as two similar-sized fragmented lobes, implying a ~300 km/s pulsar kick under symmetry assumption and confirming low-velocity hydrogen mixing in a Type II explosion.
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Identifying a circum-jet southern ring counterpart to the northern jet of the Crab Nebula
A southern circum-jet ring in the Crab Nebula is identified and attributed to a counterjet within the jittering-jets explosion mechanism framework.
- 3D Kinematic Reconstruction of the Crab Nebula That Includes the Northern Ejecta `Jet'