no code implementations • 24 Dec 2020 • S. Orlando, M. Miceli, S. Ustamujic, A. Tutone, E. Greco, O. Petruk, F. Bocchino, G. Peres
According to the most popular model for the origin of cosmic rays (CRs), supernova remnants (SNRs) are the site where CRs are accelerated.
High Energy Astrophysical Phenomena
no code implementations • 15 Dec 2020 • S. Ustamujic, S. Orlando, E. Greco, M. Miceli, F. Bocchino, A. Tutone, G. Peres
The morphology and the distribution of material observed in SNRs reflect the interaction of the SN blast wave with the ambient environment, the physical processes associated with the SN explosion and the internal structure of the progenitor star.
High Energy Astrophysical Phenomena
