Shocking Outflows in Seyfert Galaxies: An Imaging Perspective
Astrophysics
2007-05-23 v1
Abstract
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.
Cite
@article{arxiv.astro-ph/9607162,
title = {Shocking Outflows in Seyfert Galaxies: An Imaging Perspective},
author = {Richard Pogge},
journal= {arXiv preprint arXiv:astro-ph/9607162},
year = {2007}
}
Comments
4 pages with 2 embedded PostScript figures, uses aspconf.sty, epsf.sty; To appear in "Emission Lines in Active Galaxies: New Methods and Techniques", proceedings of IAU Colloquium 159, Shanghai, June 1996. eds. B.M. Peterson, F.-Z. Cheng, and A.S. Wilson (Astronomical Society of the Pacific: San Francisco)