Published in Re. Prog. Phys. 54 (1991) 579-633. Printed in the UK
Abstract. Our current knowledge of active nuclei is reviewed. The
importance of observational
data taken over a wide range of frequencies, from radio and infrared
through optical and ultraviolet to x-rays and
-rays, is
emphasized. Important overall principles
include the continuity from quasars and QSOs through Seyfert and radio
galaxies to
low-luminosity LINERs, the importance of considering roughly
cylindrically symmetric
(rather than spherically symmetric) structures, and that the various
regions generally have different axes and planes of symmetry, and are
often warped.
Table of Contents
HISTORICAL INTRODUCTION
OPTICAL SPECTRA
Classification
Diagnostics
Photoionization
Broad-line region
Accretion disk continuum
Ultraviolet line spectra
Temporal variation
Completeness of Seyfert galaxy samples
OTHER WAVELENGTH REGIONS
Radio-frequency spectral region
Infrared continuum
X-ray region
Gamma-ray radiation
TORUS MODEL
Cylindrical symmetry
Seyfert 2s with `hidden' BLRs
Ionization cones
VELOCITY FIELDS
Narrow-line profiles
Extended emission-line region
Overall NLR velocity field
BLR velocity field
Possible magnetic fields
CONTINUITY OF AGN PROPERTIES
QSOs and Seyfert 1 galaxies
Quasars and radio galaxies
Few high-luminosity Seyfert 2s
LINERs
FUELLING
Introduction
Luminosity functions of AGNs
Black holes in normal galaxies
Clusters, groups and neighbor galaxies
Interactions and mergers
EVOLUTION
Fuelling black holes
Formation rate
QSOs in formation
MISCELLANEOUS
Molecular gas
Warmers
CONCLUSION
REFERENCES