2019MNRAS.488.2466B

Query : 2019MNRAS.488.2466B

2019MNRAS.488.2466B - Mon. Not. R. Astron. Soc., 488, 2466-2472 (2019/September-2)

Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification.

BELL A.R., MATTHEWS J.H. and BLUNDELL K.M.

Abstract (from CDS):

We show that the energy required to turbulently amplify magnetic field during cosmic ray (CR) acceleration by shocks extracts energy from the CR and steepens the CR energy spectrum.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): acceleration of particles - magnetic fields - shock waves - cosmic rays

Simbad objects: 3

goto Full paper

goto View the references in ADS

Number of rows : 3
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 NAME Kepler's SN SNR 17 30 40.51 -21 29 14.4           ~ 851 3
3 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1

To bookmark this query, right click on this link: simbad:objects in 2019MNRAS.488.2466B and select 'bookmark this link' or equivalent in the popup menu