Relatore
Giacomo Principe
(Istituto Nazionale di Fisica Nucleare)
Descrizione
Taking advantage of more than 11 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 us to constrain the particle transport mechanisms and to investigate the PWN - TeV halo nature of this source
Autori principali
Giacomo Principe
(Istituto Nazionale di Fisica Nucleare)
Dr.
Alison Mitchell
(ETH Zurich)
Stefan Funk
(ECAP - Erlangen Centre for Astroparticle Physics)
Jim Hinton
(MPIK)
Sami Caroff
(PhD)
Daniel Parson
