Back to the article index
Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.SEYFERT GALAXIES AND QSOS
- 2.1.Seyfert 1s and Seyfert 2s
- 2.1.1.The emission line spectrum of Seyfert 2
galaxies
- 2.1.2.The emission line spectrum of Seyfert 1
galaxies and QSOs
- 2.1.3.Diagnostic diagrams and composite nuclear
spectra
- 2.2.The unified model
- 2.2.1.The Seyfert 1.8 and 1.9 galaxies
- 2.2.2.The X-ray properties of Seyfert 1 galaxies
- 2.2.3.The X-ray properties of Seyfert 2 galaxies
- 2.3.BALQSOs and warm absorbers
- 2.4.Fe II emission and narrow line Seyfert 1
galaxies
- 2.4.1.Fe II emission
- 2.4.2.Narrow line Seyfert 1 galaxies
- 2.5.Ultraluminous infrared galaxies
- 3.LINERS
- 3.1.Liners and AGNs
- 3.2.Liners and cooling flows
- 3.3.Liners and ULIGs
- 3.4.Emission lines in giant elliptical galaxies
- 4.RADIO GALAXIES
- 4.1.FR Is and FR IIs
- 4.2.Host galaxies of FR I and FR II radio sources
- 4.3.Emission line spectra of radio galaxies
- 4.3.1.FR II radio galaxies
- 4.3.2.FR I radio galaxies
- 4.4.Blazars
- 4.4.1.Emission line properties
- 4.4.2.Brightness temperature and variability of the core
- 4.4.3.Doppler and Lorentz factors
- 4.4.4.The dual nature of the BLLs
- 4.5.Basic differences between FR Is, FR IIs and
radio quiet AGNs
- 4.5.1.Radio loud vs. radio quiet
AGNs
- 4.5.2.FR I vs. FR II radio galaxies: the ADAF
model
- 5.RED QSOS AND TYPE 2 QSOS
- 5.1.The relative numbers of Seyfert 1 and Seyfert 2
galaxies
- 5.2.Red QSOs
- 5.3.Type 2 QSOs
- 6.CONCLUSIONS
- REFERENCES