2020A&A...638A..29B


Query : 2020A&A...638A..29B

2020A&A...638A..29B - Astronomy and Astrophysics, volume 638A, 29-29 (2020/6-1)

Radio spectral properties and jet duty cycle in the restarted radio galaxy 3C388.

BRIENZA M., MORGANTI R., HARWOOD J., DUCHET T., RAJPUROHIT K., SHULEVSKI A., HARDCASTLE M.J., MAHATMA V., GODFREY L.E.H., PRANDONI I., SHIMWELL T.W. and INTEMA H.

Abstract (from CDS):


Context. Restarted radio galaxies represent a unique tool for investigating the duty cycle of the jet activity in active galactic nuclei (AGN). The radio galaxy 3C388 has long been claimed to be a peculiar example of an AGN with multi-epoch activity because it shows a very sharp discontinuity in the GHz spectral index distribution of its lobes.
Aims. We present here for the first time a spatially resolved study of the radio spectrum of 3C388 down toMHz frequencies aimed at investigating the radiative age of the source and constraining its duty cycle.
Methods. We used new low-frequency observations at 144MHz performed with the Low Frequency Array and at 350MHz performed with the Very Large Array that we combined with archival data at higher frequencies (614, 1400, and 4850MHz).
Results. We find that the spectral indices in the lower frequency range, 144-614MHz, have flatter values (αlow∼0.55-1.14) than those observed in the higher frequency range, 1400-4850MHz, (αhigh∼0.75-1.57), but they follow the same distribution across the lobes, with a systematic steepening towards the edges. However, the spectral shape throughout the source is not uniform and often deviates from standard models. This suggests that mixing of different particle populations occurs, although it remains difficult to understand whether this is caused by observational limitations (insufficient spatial resolution and/or projection effects) or by the intrinsic presence of multiple particle populations, which might be related to the two different outbursts.
Conclusions. Using single-injection radiative models, we compute that the total source age is ≤80Myr and that the duty cycle is about ton/ttot∼60%, which is enough to prevent the intracluster medium from cooling, according to X-ray estimates. While to date the radio spectral distribution of 3C388 remains a rare case among radio galaxies, multi-frequency surveys performed with new-generation instruments will soon allow us to investigate whether more sources with the same characteristics exist.

Abstract Copyright: © ESO 2020

Journal keyword(s): galaxies: individual: 3C388 - galaxies: active - galaxies: jets - radio continuum: galaxies

VizieR on-line data: <Available at CDS (J/A+A/638/A29): list.dat fits/*>

Simbad objects: 11

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Number of rows : 11
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 NGC 326 rG 00 58 22.6298561088 +26 51 58.701156300   14.9 13     ~ 181 2
2 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2767 2
3 UGC 2489 GiC 03 01 51.4 +35 50 23           ~ 177 1
4 3C 219 Sy1 09 21 08.6258123424 +45 38 57.358202856   19.56 18.69     ~ 406 2
5 3C 286 Sy1 13 31 08.2883506368 +30 30 32.960091564   17.51 17.25     ~ 4252 2
6 3C 295 Sy2 14 11 20.6 +52 12 09   22.34 20.80 18.54   ~ 968 5
7 3C 338.0 QSO 16 28 38.24470063 +39 33 04.2335319   12.78 11.78     ~ 751 5
8 NAME Hercules A rG 16 51 07.9886687784 +04 59 35.547131472     18.25     ~ 457 1
9 ICRF J182931.7+484446 Sy1 18 29 31.7809732968 +48 44 46.160168892   17.05 16.81 16.860   ~ 676 1
10 3C 388.0 SyG 18 44 02.3840387736 +45 33 29.628672300   16.91 15.56     ~ 322 1
11 ICRF J184511.1+400751 G 18 45 11.13152826 +40 07 51.5782508   20.0       ~ 22 1

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2023.10.03-21:54:44

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