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Magnetic self-compression in laboratory plasmas, quasars and radio galaxies. Part II

Published online by Cambridge University Press:  09 March 2009

Eric J. Lerner
Eric J. Lerner
Affiliation:
20 Pine Knoll Drive, Lawrenceville, NJ 08648
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Abstract

A model of quasars and radio galaxies and their associated jets is further elaborated here. The model, presented in Part I of this paper, is based on magnetic selfcompression as the process involved in producing extremely high energy densities. In the present paper, the results derived in Part I are used to predict radiation spectra from quasars, and to extend the model to radio galaxies. The role of magnetic self-compression of magnetic vortices in the origin of filamentary superclusters of galaxies is briefly discussed.

Type
Research Article
Information
Laser and Particle Beams , Volume 4 , Issue 2 , May 1986 , pp. 215 - 222
Copyright
Copyright © Cambridge University Press 1986

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