Low-Luminosity Seyfert Nuclei

Simple item page
dc.creatorHo, Luis C.
dc.creatorFilippenko, Alexei V.
dc.creatorSargent, Wallace L. W.
dc.date1996-07-23
dc.date.accessioned2026-07-07T02:21:39Z
dc.date.available2026-07-07T02:21:39Z
dc.descriptionWe describe a new sample of Seyfert nuclei discovered during the course of an optical spectroscopic survey of nearby galaxies. The majority of the objects, many recognized for the first time, have luminosities much lower than those of classical Seyferts and populate the faint end of the AGN luminosity function. A significant fraction of the nuclei emit broad H-alpha emission qualitatively similar to the broad lines seen in classical Seyfert 1 nuclei and QSOs.
dc.descriptionTo appear in Emission Lines in Active Galaxies: New Methods and Techniques, ed. B. M. Peterson, F.-Z. Cheng, and A. S. Wilson (San Francisco: ASP), in press. LaTex, 5 pages. ASP Conference Series macros included
dc.identifierhttps://arxiv.org/abs/astro-ph/9607118
dc.identifierhttp://arxiv.org/abs/astro-ph/9607118
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10580
dc.subjectAstrophysics
dc.titleLow-Luminosity Seyfert Nuclei
dc.typetext

Files

Collections

arXiv