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Leptonic non-thermal emission from supernova remnants evolving in the circumstellar magnetic field
Iurii Sushch, Robert Brose, Martin Pohl +2
The very-high-energy (VHE; E > 100 GeV) gamma-ray emission observed from a number of Supernova remnants (SNRs) indicates particle acceleration to high energies at the shock of the…
Non-thermal emission from young supernova remnants in dense circumstellar environments
Robert Brose, Jonathan Mackey, Iurii Sushch
Supernova remnants are known to accelerate cosmic rays (CRs) on account of their non-thermal emission of radio waves, X-rays, and gamma rays. However, the ability to accelerate CRs…
Morphology of supernova remnants and their halos
Robert Brose, Martin Pohl, Iurii Sushch
Supernova remnants (SNRs) are known to accelerate particles to relativistic energies, on account of their nonthermal emission. The observational progress from radio to gamma-ray ob…