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Conference Paper

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

MPS-Authors
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Mitchell,  Alison
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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Hinton,  Jim
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Parsons,  Robert Daniel
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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Hahn,  Joachim
Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society;

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1909.11367.pdf
(Preprint), 961KB

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Citation

Principe, G., Mitchell, A., Hinton, J., Caroff, S., Parsons, R. D., Hahn, J., et al. (2019). Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by Fermi-LAT. Proceedings of Science, ICRC2019: 595. Retrieved from http://arxiv.org/abs/1909.11367.


Cite as: http://hdl.handle.net/21.11116/0000-0005-72AF-6
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.