Cargando…
High Energy Neutrino expectations from the Central Molecular Zone
The density of molecular gas in the central few hundreds parsecs of our Galaxy is estimated to be two orders of magnitude larger than the Galactic average. This, so called, Central Molecular Zone, represent a privileged target where to look for a signature of Galactic cosmic ray interactions. Here w...
| Autores principales: | , , , , , |
|---|---|
| Lenguaje: | eng |
| Publicado: |
SISSA
2018
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.22323/1.301.0939 http://cds.cern.ch/record/2672610 |