Can a single supernova remnant account for the gamma-ray emission of G106.3+2.7?
P. Cristofari, G. Emery, T. Lubrano di Vavaria, H. Costantini et autres
Context. The supernova remnant (SNR) G106.3+2.7 is a complex TeV emitting source whose emission is still poorly understood. There have been numerous discussions on its potential of being a SNR PeVatron since its gamma-ray spectra do not seem to exhibit any significant …
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