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Relationships of the Active Nucleus, Galaxy, and Environment

Published online by Cambridge University Press:  07 August 2017

K. J. Fricke  and
W. Kollatschny
K. J. Fricke
Affiliation:
Universitätssternwarte Göttingen, Geismarlandstr. 11, D-3400 Göttingen, FRG
W. Kollatschny
Affiliation:
Universitätssternwarte Göttingen, Geismarlandstr. 11, D-3400 Göttingen, FRG

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35 years ago Baade and Minkowski (1954) suggested that a galaxy collision - diagnosed from the peculiar appearance of the parent object and its strong emission lines - is responsible for the strong radio-source CygA. This was the first time that gravitational interactions between galaxies were suggested to trigger nuclear activity. Over the following decades after the detection of the quasars and the gradual realization that quasars, comparable to the Seyfert phenomenon, are events at the nuclei of seemingly isolated galaxies, the collision hypothesis was abandoned. Efforts concentrated on the understanding of the activity as internal processes in the host galaxies, possibly aided by infall of gas from the intergalactic medium (cf. Rees, 1978; Gunn, 1979).

Type
Part 8: Relationships of Nucleus, Galaxy and Environment
Information
Symposium - International Astronomical Union , Volume 134: Active Galactic Nuclei , 1989 , pp. 425 - 444
Copyright
Copyright © Kluwer 1989 

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