2018A&A...612A..19B


Query : 2018A&A...612A..19B

2018A&A...612A..19B - Astronomy and Astrophysics, volume 612A, 19-19 (2018/4-1)

The VLT/MUSE view of the central galaxy in Abell 2052. Ionized gas swept by the expanding radio source.

BALMAVERDE B., CAPETTI A., MARCONI A. and VENTURI G.

Abstract (from CDS):

We report observations of the radio galaxy 3C 317 (at z=0.0345) located at the center of the Abell cluster A2052, obtained with the VLT/MUSE integral field spectrograph. The Chandra images of this cluster show cavities in the X-ray emitting gas, which were produced by the expansion of the radio lobes inflated by the active galactic nucleus (AGN). Our exquisite MUSE data show with unprecedented detail the complex network of line emitting filaments enshrouding the northern X-ray cavity. We do not detect any emission lines from the southern cavity, with a luminosity asymmetry between the two regions higher than ∼75. The emission lines produced by the warm phase of the interstellar medium (WIM) enable us to obtain unique information on the properties of the emitting gas. We find dense gas (up to 270cm–3) that makes up part of a global quasi spherical outflow that is driven by the radio source, and obtain a direct estimate of the expansion velocity of the cavities (265km/s). The emission lines diagnostic rules out ionization from the AGN or from star-forming regions, suggesting instead ionization from slow shocks or from cosmic rays. The striking asymmetric line emission observed between the two cavities contrasts with the less pronounced differences between the north and south sides in the hot gas; this represents a significant new ingredient for our understanding of the process of the exchange of energy between the relativistic plasma and the external medium. We conclude that the expanding radio lobes displace the hot tenuous phase of the interstellar medium (ISM), but also impact the colder and denser ISM phases. These results show the effects of the AGN on its host and the importance of radio mode feedback.

Abstract Copyright: © ESO 2018

Journal keyword(s): galaxies: active - galaxies: clusters: general - galaxies: clusters: individual: A2052 - galaxies: star formation - galaxies: nuclei - galaxies: jets

VizieR on-line data: <Available at CDS (J/A+A/612/A19): list.dat fits/*>

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 UGC 9799 Sy2 15 16 44.4893939136 +07 01 17.825410740   15.19 14.17     ~ 432 3
2 ACO 2052 ClG 15 16 45.5 +07 00 01           ~ 703 1

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2022.09.27-02:35:14

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