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A radio through x-ray study of the jet/companion-galaxy interaction in 3C 321

A radio through x-ray study of the jet/companion-galaxy interaction in 3C 321
A radio through x-ray study of the jet/companion-galaxy interaction in 3C 321
We present a multiwavelength study of the nucleus, environment, jets, and hot spots of the nearby FR II radio galaxy 3C 321, using new and archival data from MERLIN, the VLA, Spitzer, HST, and Chandra. An initially collimated radio jet extends northwest from the nucleus of its host galaxy and produces a compact knot of radio emission adjacent (in projection) to a companion galaxy, after which it dramatically flares and bends, extending out in a diffuse structure 35 kpc northwest of the nucleus. We argue that the simplest explanation for the unusual morphology of the jet is that it is undergoing an interaction with the companion galaxy. Given that the northwest hot spot that lies 250 kpc from the core shows X-ray emission, which likely indicates in situ high-energy particle acceleration, we argue that the jet-companion interaction is not a steady state situation. Instead, we suggest that the jet has been disrupted on a timescale less than the light-travel time to the end of the lobe, ~106 yr, and that the jet flow to this hot spot will only be disrupted for as long as the jet-companion interaction takes place. The host galaxy of 3C 321 and the companion galaxy are in the process of merging, and each hosts a luminous AGN. As this is an unusual situation, we investigate the hypothesis that the interacting jet has driven material on to the companion galaxy, triggering its AGN. Finally, we present detailed radio and X-ray observations of both hot spots, which show that there are multiple emission sites, with spatial offsets between the radio and X-ray emission.
galaxies: active, galaxies: individual (3C 321), galaxies: jets, X-rays: galaxies
0004-637X
Evans, Daniel A.
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Fong, Wen‐Fai
a9082fd0-2668-4f3f-819d-c89e53d26791
Hardcastle, Martin J.
a6df461a-5e27-4800-a76a-b5ac8d6939f8
Kraft, Ralph P.
811e3612-4856-40dc-b9b6-c8a4812c8d25
Lee, Julia C.
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Worrall, Diana M.
48262122-f72d-492f-bd71-320f3b971f58
Birkinshaw, Mark
c1a9ef38-68b2-44fe-bb50-3f5394788f1c
Croston, Judith H.
b10aa3fb-620e-4ec2-93e5-8594748d4822
Muxlow, Tom W.B.
886c3bfd-b57a-43cd-8cd2-87f200c634e5
Evans, Daniel A.
79a05b03-53f4-4dba-aed4-ad1d50716c4b
Fong, Wen‐Fai
a9082fd0-2668-4f3f-819d-c89e53d26791
Hardcastle, Martin J.
a6df461a-5e27-4800-a76a-b5ac8d6939f8
Kraft, Ralph P.
811e3612-4856-40dc-b9b6-c8a4812c8d25
Lee, Julia C.
2bc510c5-aa01-46e5-8581-0625e8a46b7e
Worrall, Diana M.
48262122-f72d-492f-bd71-320f3b971f58
Birkinshaw, Mark
c1a9ef38-68b2-44fe-bb50-3f5394788f1c
Croston, Judith H.
b10aa3fb-620e-4ec2-93e5-8594748d4822
Muxlow, Tom W.B.
886c3bfd-b57a-43cd-8cd2-87f200c634e5

Evans, Daniel A., Fong, Wen‐Fai, Hardcastle, Martin J., Kraft, Ralph P., Lee, Julia C., Worrall, Diana M., Birkinshaw, Mark, Croston, Judith H. and Muxlow, Tom W.B. (2008) A radio through x-ray study of the jet/companion-galaxy interaction in 3C 321. Astrophysical Journal, 675 (2), [1057]. (doi:10.1086/527410).

Record type: Article

Abstract

We present a multiwavelength study of the nucleus, environment, jets, and hot spots of the nearby FR II radio galaxy 3C 321, using new and archival data from MERLIN, the VLA, Spitzer, HST, and Chandra. An initially collimated radio jet extends northwest from the nucleus of its host galaxy and produces a compact knot of radio emission adjacent (in projection) to a companion galaxy, after which it dramatically flares and bends, extending out in a diffuse structure 35 kpc northwest of the nucleus. We argue that the simplest explanation for the unusual morphology of the jet is that it is undergoing an interaction with the companion galaxy. Given that the northwest hot spot that lies 250 kpc from the core shows X-ray emission, which likely indicates in situ high-energy particle acceleration, we argue that the jet-companion interaction is not a steady state situation. Instead, we suggest that the jet has been disrupted on a timescale less than the light-travel time to the end of the lobe, ~106 yr, and that the jet flow to this hot spot will only be disrupted for as long as the jet-companion interaction takes place. The host galaxy of 3C 321 and the companion galaxy are in the process of merging, and each hosts a luminous AGN. As this is an unusual situation, we investigate the hypothesis that the interacting jet has driven material on to the companion galaxy, triggering its AGN. Finally, we present detailed radio and X-ray observations of both hot spots, which show that there are multiple emission sites, with spatial offsets between the radio and X-ray emission.

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Published date: 10 March 2008
Keywords: galaxies: active, galaxies: individual (3C 321), galaxies: jets, X-rays: galaxies

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Local EPrints ID: 151987
URI: http://eprints.soton.ac.uk/id/eprint/151987
ISSN: 0004-637X
PURE UUID: c1d0eef8-f8c4-44af-833f-0473ae2bb34a

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Date deposited: 20 May 2010 14:07
Last modified: 14 Mar 2024 01:22

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Contributors

Author: Daniel A. Evans
Author: Wen‐Fai Fong
Author: Martin J. Hardcastle
Author: Ralph P. Kraft
Author: Julia C. Lee
Author: Diana M. Worrall
Author: Mark Birkinshaw
Author: Judith H. Croston
Author: Tom W.B. Muxlow

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