PoS - Proceedings of Science
Volume 358 - 36th International Cosmic Ray Conference (ICRC2019) - GRI - Gamma Ray Indirect
Influence of cosmic ray escape on gamma-ray emission from supernova remnants
L. Ksenofontov
Full text: Not available
Abstract
On the basis of the developed nonlinear kinetic theory, calculations of the expected flux of gamma radiation from the remnant of SN 1006 are performed. Here the effects of escape of high-energy particles from the acceleration region, an arbitrary dependence on the coordinate of the enhanced magnetic field and the diffusion coefficient in the upstream of the shock are taken into account. Preliminary results of calculations are presented and compared with Fermi and H.E.S.S.
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.