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Multi - Frequency Observations of Multiple Nucleus Markarian Galaxies

Published online by Cambridge University Press:  04 August 2017

W. Kollatschny  and
K.J. Fricke
W. Kollatschny
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstr. 11, D-3400 Göttingen, F.R.G.
K.J. Fricke
Affiliation:
Universitäts-Sternwarte Göttingen, Geismarlandstr. 11, D-3400 Göttingen, F.R.G.

Abstract

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Multiple nucleus Markarian Galaxies may owe their origin to merging processes among galaxies. They may therefore be key objects for our understanding of galaxy evolution and the origin of nuclear activity. From morphological and multi-spectral data we show that these objects are in an unusually high state of dynamical and nuclear activity (starbursts, Seyfert activity) as would be expected from advanced stages of galaxy mergers.

Type
VI. Environmental Aspects of Nuclear Activity
Information
Symposium - International Astronomical Union , Volume 121: Observational Evidences of Activity of Galaxies , 1987 , pp. 377 - 383
Copyright
Copyright © Reidel 1987 

References

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