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| Query : 2022MNRAS.510.2790Z |
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
| Number of rows : 4 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | SN 1572A | SN* | 00 25 21.5 | +64 08 27 | B8 | 1254 | 1 | |||||
| 2 | IC 443 | SNR | 06 17 00.0000000 | +22 34 11.998901 | ~ | 1314 | 1 | |||||
| 3 | SNR G006.4-00.1 | SNR | 18 00 31.2011719 | -23 25 48.001099 | ~ | 782 | 1 | |||||
| 4 | SNR G034.6-00.5 | SNR | 18 56 10.650 | +01 13 21.30 | ~ | 1034 | 2 |
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