2011MNRAS.418.1208B

Query : 2011MNRAS.418.1208B

2011MNRAS.418.1208B - Mon. Not. R. Astron. Soc., 418, 1208-1216 (2011/December-1)

Cosmic ray acceleration at oblique shocks.

BELL A.R., SCHURE K.M. and REVILLE B.

Abstract (from CDS):

We show that the diffusion approximation breaks down for particle acceleration at oblique shocks with velocities typical of young supernova remnants. Higher order anisotropies flatten the spectral index at quasi-parallel shocks and steepen the spectral index at quasi-perpendicular shocks. We compare the theory with observed spectral indices.

Abstract Copyright: 2011 The Authors Monthly Notices of the Royal Astronomical Society2011 RAS

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

Simbad objects: 34

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Number of rows : 34
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 SN 2002ap SN* 01 36 23.85 +15 45 13.2   13.11 14.54     SNIc-BL 587 1
3 SN 1984L SN* 02 35 30.54 -07 09 30.3   14.0       SNIb 197 1
4 SN 2003bg SN* 04 10 59.43 -31 24 50.4     15.0     SNIc 170 1
5 SN 1987A SN* 05 35 27.98840 -69 16 11.1134           SNIIpec 5203 2
6 SNR G272.2-03.2 SNR 09 06 50 -52 07.0           SNIa 78 0
7 SN 1993J SN* 09 55 24.77476 +69 01 13.7026   10.8 12.0     SNIIb 1507 1
8 SN 2003L SN* 11 03 12.33 +11 04 38.3     16.9     SNIc 77 1
9 SNR G292.2-00.5 SNR 11 19.3 -61 28           ~ 98 1
10 SNR G296.8-00.3 SNR 11 58 30 -62 35.0           ~ 64 0
11 SN 1990B SN* 12 36 33.86 +11 14 29.9     15.75     SNIc 131 1
12 SN 1994I SN* 13 29 54.072 +47 11 30.50     12.9     SNIc 645 1
13 SN 1983N SN* 13 36 51.23 -29 54 01.7   11.7       SNIb 278 1
14 ESO 134-11 HII 14 40 29 -62 38.7           ~ 585 1
15 SNR G315.0-02.3 SNR 14 43 00 -62 30.0           ~ 376 1
16 NAME Lupus SN SNR 15 02 22.1 -42 05 49           ~ 1407 1
17 AJG 44 Psr 16 17 33.000 -51 02 00.00           ~ 552 3
18 SNR G337.2-00.7 SNR 16 39 15.0 -47 48 27           ~ 68 1
19 SNR G349.7+00.2 SNR 17 18 10.160 -37 18 53.80           ~ 196 0
20 SNR G352.7-00.1 SNR 17 27 43 -35 06.5           ~ 79 1
21 NAME Kepler's SN SNR 17 30 40.51 -21 29 14.4           ~ 851 3
22 SNR G001.9+00.3 SNR 17 48 46.02 -27 09 52.0           ~ 243 1
23 SNR G011.2-00.3 SNR 18 11 28.9 -19 25 29           ~ 305 1
24 SNR G011.2-01.1 SNR 18 14.0 -19 46           ~ 70 1
25 SNR G021.8-00.6 SNR 18 32 45 -10 08.0           ~ 137 0
26 SNR G027.3+00.0 SNR 18 41 17.8 -04 56 12           ~ 345 3
27 SNR G029.7-00.3 SNR 18 46 22.8 -02 59 47           ~ 375 2
28 SNR G031.9+00.0 SNR 18 49 16.3 -00 55 01           ~ 368 2
29 SNR G039.2-00.3 SNR 19 04 03.9 +05 26 56           ~ 204 1
30 W 49b SNR 19 11 09.5 +09 06 21           ~ 500 1
31 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
32 SNR G093.2+06.7 SNR 20 52 25 +55 19.3           ~ 87 0
33 SN 2001ig SN* 22 57 30.69 -41 02 25.9     14.5     SNIIb 190 1
34 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1

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