2017A&A...600A..65S


Query : 2017A&A...600A..65S

2017A&A...600A..65S - Astronomy and Astrophysics, volume 600A, 65-65 (2017/4-1)

Radiative age mapping of the remnant radio galaxy B2 0924+30: the LOFAR perspective.

SHULEVSKI A., MORGANTI R., HARWOOD J.J., BARTHEL P.D., JAMROZY M., BRIENZA M., BRUNETTI G., ROTTGERING H.J.A., MURGIA M., WHITE G.J., CROSTON J.H. and BRUGGEN M.

Abstract (from CDS):

We have observed the steep spectrum radio source B2 0924+30 using the LOw Frequency ARray (LOFAR) telescope. Hosted by a z=0.026 elliptical galaxy, it has a relatively large angular size of 12' (corresponding to 360 kpc projected linear size) and a morphology reminiscent of a remnant Fanaroff-Riley type II (FRII) radio galaxy. Studying active galactic nuclei (AGN) radio remnants can give us insight into the time-scales involved into the episodic gas accretion by AGNs and their dependence on the AGN host environment. The proximity of the radio galaxy allows us to make detailed studies of its radio structure and map its spectral index and radiative age distribution. We combine LOFAR and archival images to study the spectral properties at a spatial resolution of 1'. We derive low frequency spectral index maps and use synchrotron ageing models to infer ages for different regions of the source. Thus, we are able to extend the spectral ageing studies into a hitherto unexplored frequency band, adding more robustness to our results. Our detailed spectral index mapping, while agreeing with earlier lower resolution studies, shows flattening of the spectral index towards the outer edges of the lobes. The spectral index of the lobes is α140609~-1 and gradually steepens to α140609~-1.8 moving towards the inner edges of the lobes. Using radiative ageing model fitting we show that the AGN activity ceased around 50Myr ago. We note that the outer regions of the lobes are younger than the inner regions which is interpreted as a sign that those regions are remnant hotspots. We demonstrate the usefulness of maps of AGN radio remnants taken at low frequencies and suggest caution over the interpretation of spectral ages derived from integrated flux density measurements versus age mapping. The spectral index properties as well as the derived ages of B2 0924+30 are consistent with it being an FRII AGN radio remnant. LOFAR data are proving to be instrumental in extending our studies to the lowest radio frequencies and enabling analysis of the oldest source regions.

Abstract Copyright: © ESO, 2017

Journal keyword(s): galaxies: active - radio continuum: galaxies - galaxies: individual: B2 0924+30 - galaxies: individual: B2 0924+30

VizieR on-line data: <Available at CDS (J/A+A/600/A65): list.dat fits/*>

Simbad objects: 3

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Number of rows : 3
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 3C 196 Sy1 08 13 36.0561170112 +48 13 02.644966020   18.36 17.79     ~ 549 2
2 IC 2476 LIN 09 27 52.8290410824 +29 59 08.744484660   14.5       ~ 95 0
3 ZwCl 0926+3026 ClG 09 29.5 +30 13           ~ 6 0

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