IXPE detects 9.9% ± 2.5% 2-8 keV polarization from the Kes 75 PWN in one epoch, implying a toroidal field aligned with the symmetry axis, while the first epoch shows an anomalous pulse at phase 0.5 that suppresses phase-averaged polarization.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.HE 3years
2026 3representative citing papers
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.
No measurable changes in radio and X-ray emission were observed around four glitches in PSR J2229+6114, providing evidence that magnetar-like post-glitch activity is more common in high-B rotation-powered pulsars.
citing papers explorer
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Kes 75 with IXPE: Detection of Nebular X-ray Polarization and Change in Pulsar Lightcurve
IXPE detects 9.9% ± 2.5% 2-8 keV polarization from the Kes 75 PWN in one epoch, implying a toroidal field aligned with the symmetry axis, while the first epoch shows an anomalous pulse at phase 0.5 that suppresses phase-averaged polarization.
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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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No Measurable Changes in Radio and X-ray Emission Surrounding Glitches in the Young Pulsar PSR J2229+6114
No measurable changes in radio and X-ray emission were observed around four glitches in PSR J2229+6114, providing evidence that magnetar-like post-glitch activity is more common in high-B rotation-powered pulsars.