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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...
| Autores principales: | , , , , , |
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| Lenguaje: | eng |
| Publicado: |
SISSA
2018
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.22323/1.314.0014 http://cds.cern.ch/record/2314335 |