Jet-gas interactions in the seyfert galaxy markarian 78

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Main Author: M. Whittle
Format: Artículo científico
Language:en
Published: Universidad Nacional Autónoma de México 2002
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author M. Whittle
author_facet M. Whittle
contents Jet-gas interactions in the seyfert galaxy markarian 78 M. Whittle A. S. Wilson C. H. Nelson D. Rosario J. D. Silverman Física, Astronomía y Matemáticas GALAXIES: ISM GALAXIES: JETS GALAXIES: SEYFERT GALAXIES: INDIVIDUAL (MARKARIAN 78) The Seyfert 2 galaxy Markarian 78 o ers a rare opportunity to study the interaction of kpc scale radio outowswith the surrounding emission line gas. Using VLA and HST imaging and spectroscopy we identify a number ofsignatures of the interaction, including jet disruption and deection. Folding in kinematic features, we identifythree regions which may be exhibiting early, intermediate, and late stages of cloud disruption by the jet ow.Emission line ratios do not uniquely favour either photo- or shock ionization, however the lack of correlationsbetween line ratios and velocities argues against the importance of shock ionization. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101341 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.13
format Artículo científico
id redalyc_57101341
institution Redalyc
language en
publishDate 2002
publisher Universidad Nacional Autónoma de México
spellingShingle Jet-gas interactions in the seyfert galaxy markarian 78
M. Whittle
Física, Astronomía y Matemáticas
GALAXIES: ISM
GALAXIES: JETS
GALAXIES: SEYFERT
GALAXIES: INDIVIDUAL (MARKARIAN 78)
Jet-gas interactions in the seyfert galaxy markarian 78 M. Whittle A. S. Wilson C. H. Nelson D. Rosario J. D. Silverman Física, Astronomía y Matemáticas GALAXIES: ISM GALAXIES: JETS GALAXIES: SEYFERT GALAXIES: INDIVIDUAL (MARKARIAN 78) The Seyfert 2 galaxy Markarian 78 o ers a rare opportunity to study the interaction of kpc scale radio outowswith the surrounding emission line gas. Using VLA and HST imaging and spectroscopy we identify a number ofsignatures of the interaction, including jet disruption and deection. Folding in kinematic features, we identifythree regions which may be exhibiting early, intermediate, and late stages of cloud disruption by the jet ow.Emission line ratios do not uniquely favour either photo- or shock ionization, however the lack of correlationsbetween line ratios and velocities argues against the importance of shock ionization. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101341 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.13
title Jet-gas interactions in the seyfert galaxy markarian 78
topic Física, Astronomía y Matemáticas
GALAXIES: ISM
GALAXIES: JETS
GALAXIES: SEYFERT
GALAXIES: INDIVIDUAL (MARKARIAN 78)
url https://www.redalyc.org/articulo.oa?id=57101341