(2) Profile of the Non-Thermal Filaments of SNRs =>High Energy Particle Acceleration =>High Energy Particle Acceleration In all the SNRs & GC Non Thermal.
Shock acceleration of cosmic rays Tony Bell Imperial College, London.
Radio and X-Ray Properties of Magellanic Cloud Supernova Remnants
Radio and X-Ray Properties of Magellanic Cloud Supernova Remnants John R. Dickel Univ. of Illinois with: D. Milne. R. Williams, V. McIntyre, J. Lazendic,
Origin of high-energy cosmic rays Vladimir Ptuskin IZMIRAN.
Magnetic field and accelerated shock acceleration
Origin of high-energy cosmic rays Vladimir Ptuskin IZMIRAN
