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arXiv · 1909.11367

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

Giacomo Principe·Alison Mitchell·Jim Hinton·Sami Caroff·Daniel Parsons·Joachim Hahn·Stefan Funk
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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.

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Giacomo Principe, Alison Mitchell, Jim Hinton, Sami Caroff, Daniel Parsons, Joachim Hahn, Stefan Funk. 2019-09-25. Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT. https://arxiv.org/abs/1909.11367

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