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Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - GRD - Gamma Ray Direct
Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by the Fermi-LAT
G. Principe,* A. Mitchell, J. Hinton, D. Parson, S. Caroff, J. Hahn, S. Funk
*corresponding author
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Pre-published on: 2019 July 22
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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 HESS results enables a more complete picture of the nebula to emerge.
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