The very high energy gamma-ray diffuse emission from the Galactic Center

We present a novel interpretation of the gamma-ray diffuse emission in the Galactic Center (GC) and the Central Molecular Zone (CMZ) regions. This is based on a scenario assuming a harder scaling of the diffusion coefficient with rigidity in the inner Galaxy which reproduces the radial dependence of...

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Detalles Bibliográficos
Autores principales: Gaggero, Daniele, Grasso, Dario, Marinelli, Antonio, Taoso, Marco, Urbano, Alfredo, Ventura, Sofia
Lenguaje:eng
Publicado: SISSA 2018
Materias:
Acceso en línea:https://dx.doi.org/10.22323/1.314.0014
http://cds.cern.ch/record/2314335