Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT. (arXiv:1909.11367v1 [astro-ph.HE])

Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT. (arXiv:1909.11367v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Principe_G/0/1/0/all/0/1">Giacomo Principe</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mitchell_A/0/1/0/all/0/1">Alison Mitchell</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hinton_J/0/1/0/all/0/1">Jim Hinton</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Caroff_S/0/1/0/all/0/1">Sami Caroff</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Parsons_D/0/1/0/all/0/1">Daniel Parsons</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hahn_J/0/1/0/all/0/1">Joachim Hahn</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Funk_S/0/1/0/all/0/1">Stefan Funk</a>

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.

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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