Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by the $Fermi$-LAT - Archive ouverte HAL
Communication Dans Un Congrès Année : 2021

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

Giacomo Principe
  • Fonction : Auteur
Alison Mitchell
  • Fonction : Auteur
Jim Hinton
  • Fonction : Auteur
Daniel Parsons
Joachim Hahn
  • Fonction : Auteur
Stefan Funk
  • Fonction : Auteur

Résumé

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.

Dates et versions

hal-02372409 , version 1 (20-11-2019)

Identifiants

Citer

Giacomo Principe, Alison Mitchell, Jim Hinton, Daniel Parsons, Sami Caroff, et al.. Energy-dependent morphology of the pulsar wind nebula HESS J1825-137 seen by the $Fermi$-LAT. 36th International Cosmic Ray Conference, Jul 2019, Madison, United States. pp.595, ⟨10.22323/1.358.0595⟩. ⟨hal-02372409⟩
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