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Relationships Between Seyfert Galaxies, QSOs, and BL LACs

Published online by Cambridge University Press:  04 August 2017

J.B. Hutchings
J.B. Hutchings*
Affiliation:
Dominion Astrophysical Observatory, 5071 W. Saanich Rd, Victoria, B.C., Canada

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In this review, I will deal principally with the optical morphology of these three types of object, and attempt to outline similarities and essential differences. By this, I mean to include studies of the types of host galaxy, nuclear and galaxy luminosities and colours, interactions with other galaxies, and the general associations with other galaxies. Where relevant, I will refer to morphology at other wavelengths (generally radio), spectroscopy, and UV or X-ray properties. However, I expect these areas to be covered much more fully by other reviews and papers in this volume.

Type
VI. Environmental Aspects of Nuclear Activity
Information
Symposium - International Astronomical Union , Volume 121: Observational Evidences of Activity of Galaxies , 1987 , pp. 349 - 361
Copyright
Copyright © Reidel 1987 

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