SIMBAD references

2022MNRAS.510.2790Z - Mon. Not. R. Astron. Soc., 510, 2790-2796 (2022/February-3)

Role of the radiative stage for cosmic ray acceleration in SNRs.

ZIRAKASHVILI V.N. and PTUSKIN V.S.

Abstract (from CDS):

We consider diffusive shock acceleration in supernova remnants throughout their evolution including a radiative stage. It is found that a more efficient acceleration and fast exit of particles at the radiative stage results in the hardening of the source cosmic ray proton and electron spectra at energies ∼100-500 GeV. The effect is stronger for cosmic ray electrons.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): acceleration of particles - shock waves - ISM: supernova remnants

Simbad objects: 4

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