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AGN as a Result of Evolution of Binary Gravimagnetic Rotators

Published online by Cambridge University Press:  19 July 2016

Olga K. Sil'chenko  and
Vladimir M. Lipunov
Olga K. Sil'chenko
Affiliation:
Sternberg Astronomical Institute, Universitetskij pr., 13, 119899 Moscow, Russia
Vladimir M. Lipunov
Affiliation:
Sternberg Astronomical Institute, Universitetskij pr., 13, 119899 Moscow, Russia Faculty of Physics, Moscow University, Leninskie Gory, 117234 Moscow, Russia

Extract

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Supermassive black holes in AGN can form directly as the results of collapse of supermassive magnetic and rotating stars (gravimagnetic rotators). In this case naturally we can consider the binary magnetic rotator systems as progenitors of active galactic nuclei. One of the most important consequence of this scenario is an existence of moving galactic nuclei, so called “nomadic” nuclei.

Type
Poster contributions: Statistical Studies and Evolution
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 521
Copyright
Copyright © Kluwer 1994 

References

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