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Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT

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arxiv 1909.11367 v1 pith:O6NFWPY5 submitted 2019-09-25 astro-ph.HE

Giacomo Principe , Alison Mitchell , Jim Hinton , Sami Caroff , Daniel Parsons , Joachim Hahn , Stefan Funk This is my paper · ORCID
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keywords analysishessj1825-137nebulafermi-latpulsarresultswind
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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.

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