Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-29T14:14:24.202Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Get access Rights & Permissions [Opens in a new window]

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

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Bridle, A. H. et al. 1979 Ast. and Astrophys. 86, 201.Google Scholar
Hoyle, R. et al. 1966 Nature, 205, 751.CrossRefGoogle Scholar
Moffatt, H. H. 1970 J. Fluid Mech. 41, 435.CrossRefGoogle Scholar
Pouquet, A. & Patterson, G. S. 1978 J. Fluid Mech. 35, 305.CrossRefGoogle Scholar
Rudnick, L. 1981 Extragalactic Radio Ast. Proc. IAU Sym. #97.Google Scholar
Steenbeck, M. et al. 1966 Z. Nature, 21a, 369.Google Scholar
Wittels, J. J. et al. 1982 Ap. J. 262, 127.CrossRefGoogle Scholar
Yusef-Zadeh, et al. , 1984 Nature, 310, 557.CrossRefGoogle Scholar