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High-resolution observations of the pulsar wind nebula in supernova remnant G11.2−0.3 reveal a radio jet with a helical magnetic field, suggesting complex particle acceleration mechanisms. doi.org/g874nn
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Radio Observation of the Pulsar Wind Nebula in SNR G11.2-0.3 https://arxiv.org/pdf/2503.01802 Yu Zhang, Yihan Liu, C.-Y. Ng, Mallory S. E. Roberts, Lili Yang.
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helical B-field inside the jet, the equipartition B-field strength of which is below 100\,$\mu$G. [5/5 of https://arxiv.org/abs/2503.01802v1]
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and -0.10, respectively. Meanwhile for the jet region, the spectral break between radio and X-ray spectra implies particle acceleration mechanisms other than a diffusive shock acceleration. Polarization results suggest a [4/5 of https://arxiv.org/abs/25…