56 citations · 96 across the 7 of their papers we have counts for
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astro-ph.HE2023
Magnetic Field Structure of the Crab Pulsar Wind Nebula Revealed with IXPE
T. Mizuno, H. Ohno, E. Watanabe +5
We report a detailed study of the magnetic-field structure of the Crab pulsar wind nebula, using the X-ray polarization data in 2--8~keV obtained with the Imaging X-ray Polarimetry…
astro-ph.HE2023★ 56 cited
Vela pulsar wind nebula x-rays are polarized to near the synchrotron limit
Fei Xie, Alessandro Di Marco, Fabio La Monaca +90
Pulsar wind nebulae are formed when outflows of relativistic electrons and positrons hit the surrounding supernova remnant or interstellar medium at a shock front. The Vela pulsar…