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Shocking Outflows in Seyfert Galaxies: An Imaging Perspective

Published online by Cambridge University Press:  12 April 2016

Richard W. Pogge
Richard W. Pogge*
Affiliation:
Department of Astronomy, The Ohio State University, 174 W. 18th Ave, Columbus, OH 43210-1106, USA

Abstract

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Representative results of a search for structures suggestive of shocked gas in the circumnuclear regions of Seyfert galaxies are presented. At issue is whether we can identify regions that appear to be shocked by outflows from the active nucleus. Such regions will be good targets for future spectrophotometric studies to determine what role shocks play in the physics of the AGN/host-galaxy interaction.

Information

Type
VII. Shocks and Photoionization
Information
International Astronomical Union Colloquium , Volume 159: Emission Lines in Active Galaxies: New Methods and Techniques , 1997 , pp. 378 - 381
Copyright
Copyright © Astronomical Society of the Pacific 1997

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