2013MNRAS.430.2137K


Query : 2013MNRAS.430.2137K

2013MNRAS.430.2137K - Mon. Not. R. Astron. Soc., 430, 2137-2153 (2013/April-2)

Episodic radio galaxies J0116-4722 and J1158+2621: can we constrain the quiescent phase of nuclear activity ?

KONAR C., HARDCASTLE M.J., JAMROZY M. and CROSTON J.H.

Abstract (from CDS):

We present multifrequency radio observations of two well-known episodic Fanaroff-Railey type II (FR II) radio galaxies (J0116-4722 and J1158+2621) and a detailed investigation of the life cycle of episodic radio galaxies from their spectral and radiative properties. Combining our previous work with the present results, we either constrain or place very good limits on the active and quiescent phases of a small sample of episodic FR II radio galaxies. The duration of the quiescent phase can be as small as the hotspot fading time of the previous episode, and as high as a few tens of Myr; however, for none of the sources in our sample is it close to the duration of the active phase of the previous episode. We also find that for many episodic radio galaxies, the nucleus is variable at radio wavelengths. For our small sample of seven episodic radio galaxies, we find four to have strongly variable cores, a much larger proportion than is generally found in samples of normal FR II radio galaxies. Studies with larger samples will be required to establish a statistical association between core variability and episodic radio activity.

Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)

Journal keyword(s): galaxies: active - galaxies: individual: J0116-4722 - galaxies: individual: J1158+2621 - galaxies: nuclei - radio continuum: galaxies

CDS comments: J1159+3224 is a misprint for J1158+2621.

Simbad objects: 23

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Number of rows : 23
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 4C 32.04 rG 00 41 46.6 +32 25 09           ~ 25 2
2 NGC 315 LIN 00 57 48.88334410 +30 21 08.8119345 12.80 12.20 11.16 11.26   ~ 790 2
3 PKS 0114-47 rG 01 16 25.0503696336 -47 22 41.107795248   16.5 16.5     ~ 63 1
4 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2820 2
5 3C 79.0 Sy2 03 10 00.0936589848 +17 05 58.599361932   19.54 18.75     ~ 258 3
6 4C 14.11 Rad 04 14 27.6 +14 16 56           ~ 16 0
7 LEDA 2819197 G 04 14 29.808149 +14 16 23.48209           ~ 74 1
8 ICRF J054236.1+495107 Sy1 05 42 36.13789710 +49 51 07.2337139   18.45 17.80 17.210   ~ 1499 1
9 ICRF J081950.5+753839 Sy2 08 19 50.5199667840 +75 38 39.541356024     17.50     ~ 20 0
10 Z 150-14 Sy2 08 40 02.336 +29 49 02.73   20.00 19.62     ~ 193 1
11 NAME Hya A LIN 09 18 05.66848602 -12 05 43.8060823   14.38 14.8     ~ 1014 1
12 [KJB2018] GRS J0929+4146 rG 09 29 10.660 +41 46 45.59           ~ 22 1
13 4C 26.35 LIN 11 58 20.138 +26 21 12.08     18.5     ~ 58 2
14 4CT 74.17.1 Rad 12 11 38 +74 19.4           ~ 14 0
15 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7223 3
16 NAME Centaurus A Sy2 13 25 27.61521044 -43 01 08.8050291   8.18 6.84 6.66   ~ 4495 3
17 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4353 2
18 4C 33.33 rG 14 53 02.8682754912 +33 08 42.450468612           ~ 48 3
19 PKS 1545-321 rG 15 48 58.0331477149 -32 16 58.157614838           ~ 49 1
20 NGC 6251 Sy2 16 32 31.96989253 +82 32 16.3999044 15.24 14.66 12.89 7.62   ~ 731 0
21 NAME Hercules A rG 16 51 07.9886687784 +04 59 35.547131472     18.25     ~ 467 1
22 8C 1834+620 Sy2 18 35 10.920 +62 04 08.14           ~ 49 2
23 3C 388.0 SyG 18 44 02.3840387736 +45 33 29.628672300   16.91 15.56     ~ 326 1

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