Linear radio structures in selected Seyfert and LINER galaxies

E. Xanthopoulos; A.H. Thean; A. Pedlar; A.M.S. Richards

doi:10.1063/1.2348035

Linear radio structures in selected Seyfert and LINER galaxies

E. Xanthopoulos, A.H. Thean, A. Pedlar, A.M.S. Richards

Research output: Chapter in Book/Conference proceeding › Conference contribution

Abstract

High resolution MERLIN 5 GHz observations (0″.04) of 7 Seyfert galaxies, selected as the ones previously showing evidence of collimated ejection, have been compared with high resolution archive HST data. The radio maps reveal rich structures in all the galaxies. NGC 2639 and TXFS 2226-184 have multiple knot parsec-scale extended structures, Mrk 1034, Mrk 1210, NGC 4922C and NGC 5506 reveal one-sided jets, while IC 1481 exhibits a jet-like extension. The close correlation between the radio-emitting relativistic plasma and the ionized gas in the inner regions of these galaxies allows us to study in detail the physics close to the center of low luminosity AGN. © 2006 American Institute of Physics.

Original language	Undefined
Title of host publication	AIP Conference Proceedings
Pages	592-596
Number of pages	5
Volume	848
DOIs	https://doi.org/10.1063/1.2348035
Publication status	Published - 2006
Event	7th International Conference of the Hellenic Astronomical Society - Lixourion, Kefallinia Island, Greece Duration: 8 Sept 2005 → 11 Sept 2005

Conference

Conference	7th International Conference of the Hellenic Astronomical Society
Country/Territory	Greece
City	Lixourion, Kefallinia Island
Period	8/09/05 → 11/09/05

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10.1063/1.2348035

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title = "Linear radio structures in selected Seyfert and LINER galaxies",

abstract = "High resolution MERLIN 5 GHz observations (0″.04) of 7 Seyfert galaxies, selected as the ones previously showing evidence of collimated ejection, have been compared with high resolution archive HST data. The radio maps reveal rich structures in all the galaxies. NGC 2639 and TXFS 2226-184 have multiple knot parsec-scale extended structures, Mrk 1034, Mrk 1210, NGC 4922C and NGC 5506 reveal one-sided jets, while IC 1481 exhibits a jet-like extension. The close correlation between the radio-emitting relativistic plasma and the ionized gas in the inner regions of these galaxies allows us to study in detail the physics close to the center of low luminosity AGN. {\textcopyright} 2006 American Institute of Physics.",

author = "E. Xanthopoulos and A.H. Thean and A. Pedlar and A.M.S. Richards",

year = "2006",

doi = "10.1063/1.2348035",

language = "Undefined",

isbn = "9780735403437",

volume = "848",

pages = "592--596",

booktitle = "AIP Conference Proceedings",

note = "7th International Conference of the Hellenic Astronomical Society ; Conference date: 08-09-2005 Through 11-09-2005",

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TY - GEN

T1 - Linear radio structures in selected Seyfert and LINER galaxies

AU - Xanthopoulos, E.

AU - Thean, A.H.

AU - Pedlar, A.

AU - Richards, A.M.S.

PY - 2006

Y1 - 2006

N2 - High resolution MERLIN 5 GHz observations (0″.04) of 7 Seyfert galaxies, selected as the ones previously showing evidence of collimated ejection, have been compared with high resolution archive HST data. The radio maps reveal rich structures in all the galaxies. NGC 2639 and TXFS 2226-184 have multiple knot parsec-scale extended structures, Mrk 1034, Mrk 1210, NGC 4922C and NGC 5506 reveal one-sided jets, while IC 1481 exhibits a jet-like extension. The close correlation between the radio-emitting relativistic plasma and the ionized gas in the inner regions of these galaxies allows us to study in detail the physics close to the center of low luminosity AGN. © 2006 American Institute of Physics.

AB - High resolution MERLIN 5 GHz observations (0″.04) of 7 Seyfert galaxies, selected as the ones previously showing evidence of collimated ejection, have been compared with high resolution archive HST data. The radio maps reveal rich structures in all the galaxies. NGC 2639 and TXFS 2226-184 have multiple knot parsec-scale extended structures, Mrk 1034, Mrk 1210, NGC 4922C and NGC 5506 reveal one-sided jets, while IC 1481 exhibits a jet-like extension. The close correlation between the radio-emitting relativistic plasma and the ionized gas in the inner regions of these galaxies allows us to study in detail the physics close to the center of low luminosity AGN. © 2006 American Institute of Physics.

UR - http://www.scopus.com/inward/record.url?eid=2-s2.0-33846513980&partnerID=MN8TOARS

U2 - 10.1063/1.2348035

DO - 10.1063/1.2348035

M3 - Conference contribution

SN - 9780735403437

VL - 848

SP - 592

EP - 596

BT - AIP Conference Proceedings

T2 - 7th International Conference of the Hellenic Astronomical Society

Y2 - 8 September 2005 through 11 September 2005

ER -

Linear radio structures in selected Seyfert and LINER galaxies

Abstract

Conference

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