Low-Luminosity Seyfert Nuclei
Astrophysics
2007-05-23 v1
Abstract
We 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.
Cite
@article{arxiv.astro-ph/9607118,
title = {Low-Luminosity Seyfert Nuclei},
author = {Luis C. Ho and Alexei V. Filippenko and Wallace L. W. Sargent},
journal= {arXiv preprint arXiv:astro-ph/9607118},
year = {2007}
}
Comments
To 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