Monitoring of active galactic nuclei: the why and the how.

Details Monitoring of active galactic nuclei: the why and the how. Monitoring of active galactic nuclei: the why and the how.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995msngr..80...25a&link_type=abstract

The Messenger, vol. 80, p. 25-28

Physics

3

Active Galactic Nuclei: Surveys

Scientific paper

Over the past twenty years, groundbased optical observations as well as ultraviolet, X-ray, and g-ray observations from space-borne telescopes have revealed the variable nature of the continuum and emission lines in the spectra of active galactic nuclei (hereafter referred to as AGN). Variability is now recognized as one of the distinctive features of these important but poorly understood objects.

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