2017A&A...608A..58T


Query : 2017A&A...608A..58T

2017A&A...608A..58T - Astronomy and Astrophysics, volume 608A, 58-58 (2017/12-1)

Narrow head-tail radio galaxies at very high resolution.

TERNI DE GREGORY B., FERETTI L., GIOVANNINI G., GOVONI F., MURGIA M., PERLEY R.A. and VACCA V.

Abstract (from CDS):

Aims. Narrow-angle tailed (NAT) sources in clusters of galaxies can show on the large scale very narrow tails that are unresolved even at arcsecond resolution. These sources could therefore be classified as one-sided jets. The aim of this paper is to gain new insight into the structure of these sources, and establish whether they are genuine one-sided objects, or if they are two-sided sources.
Methods. We observed a sample of apparently one-sided NAT sources at subarcsecond resolution to obtain detailed information on their structure in the nuclear regions of radio galaxies.
Results. Most radio galaxies are found to show two-sided jets with sharp bends, and therefore the sources are similar to the more classical NATs, which are affected by strong projection effects.

Abstract Copyright: © ESO, 2017

Journal keyword(s): galaxies: clusters: general - intergalactic medium - radio continuum: general - X-rays: general - X-rays: general

Simbad objects: 29

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Number of rows : 29
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 4C 31.06B BiC 01 57 16.2726263928 +32 14 47.542188624           ~ 28 1
2 ACO 278 ClG 01 57 18 +32 13.6           ~ 70 0
3 IC 310 rG 03 16 42.9787569912 +41 19 29.615579544   14.3       ~ 254 2
4 ACO 426 ClG 03 19 47.2 +41 30 47           ~ 2135 1
5 NVSS J045417+025533 Rad 04 54 17.0 +02 55 32           ~ 3 1
6 ACO 520 ClG 04 54 19.0 +02 56 49           ~ 416 0
7 [CGH98] J0455+0255B Rad 04 54 21.1 +02 55 02           ~ 2 0
8 ICRF J052109.8+163822 Sy1 05 21 09.8855216664 +16 38 22.054553988   19.37 18.84 18.480   ~ 815 1
9 QSO B0521-365 BLL 05 22 57.9841341216 -36 27 30.847204512   15.26 14.62 14.48   ~ 787 2
10 ACO 869 ClG 09 46 11 +02 21.1           ~ 13 0
11 SDSS J094613.82+022246.9 rG 09 46 13.8267635424 +02 22 47.060689404           ~ 8 0
12 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4142 2
13 NVSS J134150+262223 Rad 13 41 50.4 +26 22 12           ~ 10 1
14 ACO 1775 ClG 13 41 55.6 +26 21 53           ~ 287 0
15 [LO95] 1346+268B Rad 13 48 59.02 +26 33 36.6           ~ 5 0
16 ACO 1795 ClG 13 49 00.5 +26 35 07           ~ 1209 0
17 2MASX J15581435+2716191 rG 15 58 14.3093579688 +27 16 19.571108448           ~ 12 0
18 ACO 2142 ClG 15 58 20.00 +27 14 00.3           ~ 722 0
19 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3416 1
20 4C 39.49 BLL 16 53 52.2160772976 +39 45 36.613228860 14.09 14.15 13.29 8.26   ~ 2049 2
21 2MASX J17005206+7841214 GiC 17 00 52.2251220528 +78 41 21.123626136   16.78       ~ 23 0
22 2MASX J17033002+7839536 GiC 17 03 30.0542270136 +78 39 54.244656504   17.57       ~ 32 0
23 ACO 2256 ClG 17 03 43.5 +78 43 03           ~ 859 1
24 2MASX J17120908-2328263 G 17 12 09.0607726464 -23 28 26.650191432           ~ 12 0
25 NAME Oph Cluster ClG 17 12 24.7 -23 21 01           ~ 260 0
26 ACO 2255 ClG 17 12 50.04 +64 03 10.6           ~ 537 0
27 2MASX J17130384+6407014 rG 17 13 03.7806794784 +64 07 01.673867568           ~ 28 0
28 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 13304 0
29 UGC 12064 AGN 22 31 20.5885689288 +39 21 29.593072404   14.6       ~ 428 1

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2022.11.28-09:23:56

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