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Strong magnetic fields, galaxy formation, and the Galactic engineThe strong-magnetic-field model proposed as an energy source for AGN and quasars by Greyber (1961, 1962, 1964, 1967, 1984, 1988, and 1989) is discussed. The basic principles of the model are reviewed; its advantages (in explaining the observed features of AGN and quasars) over models based on a rotating accretion disk are indicated in a table; and its implications for galaxy and quasar formation are explored. The gravitationally bound current loops detected in nearby spiral galaxies are interpreted as weak remnants of the current loops present during their formation. An observational search for a similar loop near the Galactic center is proposed.
Document ID
19900058506
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Greyber, Howard D.
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: New York Academy of Sciences, Annals
Volume: 571
ISSN: 0077-8923
Subject Category
Astrophysics
Accession Number
90A45561
Distribution Limits
Public
Copyright
Other

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