2 papers
astro-ph.HE2026
Can a single supernova remnant account for the gamma-ray emission of G106.3+2.7?
P. Cristofari, G. Emery, T. Lubrano di Vavaria +4
SNR G106.3+2.7 is a complex TeV emitting source whose emission is still poorly understood. It has especially been at the center of numerous discussions on its potential for being a…
astro-ph.HE2026
Very High Energy Gamma Rays from Ultra Fast Outflows
B. Le Nagat Neher, E. Peretti, P. Cristofari +1
Context. Ultra fast outflows (UFOs) from active galactic nuclei (AGN) are expected to lead to the formation of sub-relativistic strong shocks expanding in a dense circumnuclear med…