2000 character limit reached
Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT (1909.11367v1)
Published 25 Sep 2019 in astro-ph.HE
Abstract: Taking advantage of 10 years of Fermi-LAT data, we perform a new and deep analysis of the pulsar wind nebula (PWN) HESS J1825-137. We present the results of the spectral analysis and of the first energy-resolved morphological study of the PWN HESS J1825-137 from 1 GeV to 1 TeV. This PWN is an archetypal system making it a perfect laboratory for studying particle transport mechanisms. Combining this analysis with recent H.E.S.S. results enables a more complete picture of the nebula to emerge.