2008MNRAS.385.1884B

Query : 2008MNRAS.385.1884B

2008MNRAS.385.1884B - Mon. Not. R. Astron. Soc., 385, 1884-1892 (2008/April-3)

Cosmic ray acceleration by a supernova shock in a dense circumstellar plasma.

BELL A.R.

Abstract (from CDS):

Cosmic ray acceleration may occur at a supernova shock expanding into a circumstellar wind sustaining a Parker spiral magnetic field. Cosmic rays drift to the poles producing a large cosmic ray pressure which can generate polar density cavities through which cosmic rays escape upstream of the shock. This may be relevant to gamma-ray bursts accompanying shock breakout.

Abstract Copyright: ©2008 The Author. Journal compilation © 2008 RAS

Journal keyword(s): shock waves - cosmic rays - supernova remnants - gamma-rays: bursts

Simbad objects: 4

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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 2006gy SN* 03 17 27.06 +41 24 19.5       14.20   SNIIn 372 1
2 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
3 HD 50896 WR* 06 54 13.0439608392 -23 55 42.023319852 5.74 6.63 6.91 7.74   WN4b 794 0
4 SN 2005ap SN* 13 01 14.84 +27 43 31.4       18.20   SLSN-I 146 1

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