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Towards a better understanding of AGN

Towards a Better Understanding of Active Galactic Nuclei


Paolo Padovani

Original Version: `New Horizons from Multi-Wavelength Sky Surveys', B. McLean et al. eds., p. 257.

Text copyright (c) 1998: Kluwer Academic Publishers

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Abstract

Active Galactic Nuclei (AGN) are ideal sources for multi-wavelength studies as their emission can cover almost 20 orders of magnitude in frequency from the radio to the gamma-ray band. After reviewing their basic properties, I will assess how well we know the multifrequency spectra of AGN as a class. I will then briefly illustrate how currently available and forthcoming sky surveys will help in addressing some of the open questions of AGN studies. Finally, an analysis of the problem of the missing Type 2 QSO will exemplify the dangers of monochromatic sky surveys for AGN.

Available files:

  • TeX file of the paper (requires crckapb.sty and psfig.tex)
  • Postscript versions of:
  • Figure 1 (65kb)
  • Figure 2 (23kb)
  • Whole paper including figures: postscript file (187kb), gzipped version (59kb)
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