Shocking Outflows in Seyfert Galaxies: An Imaging Perspective

dc.creatorPogge, Richard
dc.date1996-07-30
dc.date.accessioned2026-07-07T02:21:41Z
dc.date.available2026-07-07T02:21:41Z
dc.descriptionRepresentative 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.
dc.description4 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)
dc.identifierhttps://arxiv.org/abs/astro-ph/9607162
dc.identifierhttp://arxiv.org/abs/astro-ph/9607162
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10594
dc.subjectAstrophysics
dc.titleShocking Outflows in Seyfert Galaxies: An Imaging Perspective
dc.typetext

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