Abstract
I have been invited to present a brief review of optical, infrared and ultraviolet observations of activity nuclei. I will only describe a small sub-set of these observations, in particular those which I believe are most likely to be important in elucidating those properties of the central energy source to which we attribute the origin of all high energy phenomena. I will therefore restrict my remarks to certain aspects of BL LAc objects, optically violently variable quasars, quasars, Seyfert I galaxies and broad line radio galaxies. If we could understand these systems, we should be able to account for most other types of active nuclei, the Seyfert II galaxies, narrow line radion galaxies, all other types of Markarian galaxy, compact blue galaxy, etx. In my view, the recent observations of NGC 4151 provide us with a benchmark against which we should measure all other observations of activity nuclei.
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Pacini, F. et al. (1983). Active Galactic Nuclei. In: West, R.M. (eds) Highlights of Astronomy. International Astronomical Union / Union Astronomique Internationale, vol 6. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7110-3_9
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