2004MNRAS.347..508G


Query : 2004MNRAS.347..508G

2004MNRAS.347..508G - Mon. Not. R. Astron. Soc., 347, 508-540 (2004/January-2)

The depolarization properties of powerful radio sources: breaking the radio power versus redshift degeneracy.

GOODLET J.A., KAISER C.R., BEST P.N. and DENNETT-THORPE J.

Abstract (from CDS):

We define three samples of extragalactic radio sources of Fanaroff-Riley type II, containing 26 objects in total. The control sample consists of 6C and 7C sources with radio powers of around 1027 W/Hz at 151 MHz and redshifts of z ∼ 1. The other samples contain 3CRR sources either with comparable redshifts but radio powers about a decade larger or with comparable radio powers but redshifts around z ∼ 0.4. We use these samples to investigate the possible evolution of their depolarization and rotation measure properties with redshift and radio power independently. We used VLA data for all sources at ∼4800 MHz and two frequencies within the 1400-MHz band, either from our own observations or from the archive. We present maps of the total intensity flux, polarized flux, depolarization, spectral index, rotation measure and magnetic field direction where not previously published. Radio cores were detected in 12 of the 26 radio sources. Of the sources, 14 show a strong Laing-Garrington effect, but almost all of the sources show some depolarization asymmetry. All sources show evidence for an external Faraday screen being responsible for the observed depolarization. We find that sources at higher redshift are more strongly depolarized. Rotation measure shows no trend with either redshift or radio power. However, variations in the rotation measure across individual sources increase with the redshift of the sources but do not depend on their radio power.

Abstract Copyright: 2004 RAS

Journal keyword(s): magnetic fields - polarization - galaxies: active - galaxies: jets

Simbad objects: 26

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Number of rows : 26
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 3C 16 rG 00 37 44.570 +13 19 55.00   21       ~ 128 3
2 3C 42 rG 01 28 30.332 +29 02 59.45   20       ~ 145 1
3 3C 46 rG 01 35 24.67 +37 53 47.0   19.5       ~ 136 2
4 3C 65 rG 02 23 43.190 +40 00 52.46   23.0       ~ 185 1
5 7C 022927.30+341049.00 QSO 02 32 28.8769824336 +34 23 46.713498468   20.70 19     ~ 197 1
6 4C 14.27 Sy1 08 35 03.62136 +14 11 48.7212   19.5       ~ 59 2
7 NVSS J094618+394418 rG 09 46 18.888 +39 44 17.97           ~ 32 1
8 NVSS J101412+361727 rG 10 14 12.898 +36 17 25.18   21.5       ~ 32 1
9 4C 37.27B rG 10 21 15.795 +37 14 55.71   20.2       ~ 22 1
10 3C 252.0 rG 11 11 31.960 +35 40 44.64   22       ~ 127 1
11 4C 37.31 rG 11 32 35.913 +36 54 12.30   23       ~ 40 1
12 3C 265.0 Sy1 11 45 28.95577 +31 33 47.2434   20.0       ~ 250 1
13 3C 267 rG 11 49 56.526 +12 47 18.95   22.5       ~ 158 2
14 3C 268.1 rG 12 00 20.53 +73 00 45.7   22       ~ 149 1
15 7C 125441.29+473632.00 SyG 12 56 57.485 +47 20 20.23   22.0       ~ 285 1
16 NVSS J125905+363158 rG 12 59 05.920 +36 31 57.50           ~ 32 1
17 NVSS J125929+361704 rG 12 59 30.00936 +36 17 02.6304           ~ 29 1
18 3C 299 rG 14 21 05.6960 +41 44 49.260   20.496 19.330 18.560   ~ 187 1
19 3C 324.0 Sy1 15 49 49.170 +21 25 39.50   21.5       ~ 312 1
20 3C 341 rG 16 28 04.049 +27 41 43.07   19       ~ 146 1
21 8C 1704+608 Bla 17 04 41.3742408840 +60 44 30.520617000   15.65 15.40 15.30   ~ 782 1
22 4C 16.49 QSO 17 34 42.6025956120 +16 00 32.342065776     18.4     ~ 78 2
23 ICRF J174606.6+642149 SyG 17 46 06.67804118 +64 21 49.6602105           ~ 25 1
24 7C 1801+6902 QSO 18 01 14.6349395592 +69 02 43.771807248     19.4     ~ 22 1
25 7C 181302.70+684641.00 QSO 18 12 44.2211877336 +68 47 35.500328844     19.70     ~ 19 1
26 3C 457 QSO 23 12 07.590 +18 45 41.51   19.5       ~ 95 1

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