Prefer a chat interface with context about you and your work?
Deep<i>Chandra</i>Observation of the Pulsar Wind Nebula Powered by Pulsar PSR J1846โ0258 in the Supernova Remnant KES 75
We present the results of detailed spatial and spectral analysis of the pulsar wind nebula (PWN) in supernova remnant Kes 75 (G29.7-0.3) using a deep exposure with Chandra X-ray observatory. The PWN shows a complex morphology with clear axisymmetric structure. We identified a one-sided jet and two bright clumps aligned โฆ