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Symmetric Ejection of Massive Objects from Galactic Nuclei

Published online by Cambridge University Press:  14 August 2015

M. J. Valtonen
M. J. Valtonen*
Affiliation:
Institute of Astronomy, Cambridge, England Research Institute for Theoretical Physics, Helsinki, Finland

Abstract

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It is shown that massive objects can be ejected symmetrically in two opposite directions from the nucleus of a giant elliptical galaxy only under special initial conditions. A way of obtaining these conditions is outlined, and the resulting picture of evolution of galactic nuclei, including a quasar or a Seyfert galaxy phase, is shown to be compatible with observations.

Type
Part III/Nuclei
Information
Symposium - International Astronomical Union , Volume 69: Dynamics of Stellar Systems , 1975 , pp. 395 - 403
Copyright
Copyright © Reidel 1975 

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