Energy-dependent morphology of the pulsar wind 1 nebula HESS J1825-137 seen by Fermi-LAT
Principe G, Mitchell AM, Hinton J, Parsons RD, Caroff S, Hahn J, Funk S (2021)
Publication Type: Conference contribution
Publication year: 2021
Journal
Publisher: Sissa Medialab Srl
Book Volume: 358
Conference Proceedings Title: Proceedings of Science
Event location: Madison, WI, USA
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.
Authors with CRIS profile
Involved external institutions
National Institute for Astrophysics / Istituto Nazionale Astrofisica (INAF)
Italy (IT)
University of Zurich / Universität Zürich (UZH)
Switzerland (CH)
Max-Planck-Institut für Kernphysik (MPIK) / Max Planck Institute for Nuclear Physics
Germany (DE)
Sorbonne Université
France (FR)
Italy (IT)
University of Zurich / Universität Zürich (UZH)
Switzerland (CH)
Max-Planck-Institut für Kernphysik (MPIK) / Max Planck Institute for Nuclear Physics
Germany (DE)
Sorbonne Université
France (FR)
How to cite
APA:
Principe, G., Mitchell, A.M., Hinton, J., Parsons, R.D., Caroff, S., Hahn, J., & Funk, S. (2021). Energy-dependent morphology of the pulsar wind 1 nebula HESS J1825-137 seen by Fermi-LAT. In Proceedings of Science. Madison, WI, USA: Sissa Medialab Srl.
MLA:
Principe, G., et al. "Energy-dependent morphology of the pulsar wind 1 nebula HESS J1825-137 seen by Fermi-LAT." Proceedings of the 36th International Cosmic Ray Conference, ICRC 2019, Madison, WI, USA Sissa Medialab Srl, 2021.
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