The Magnetodynamic Model of Quasars
release_fsfyjx4g7rhflb7mlkozyh4q4m
by
L.M. Ozernoj
Abstract
Although the energy problem is one of the main difficulties of the cosmological interpretation of quasar red-shifts, there is no need to go beyond conventional physical laws in seeking an explanation. Various proposals have been made which differ in important details. I believe a suitable basis for a theory of quasars to be a supermassive plasma configuration, the matter of which is in mostly regular motion in a magnetic field. Such a magnetodynamic configuration I shall call a 'magnetoid'. On this model a quasar is a galaxy with a dense non-stellar nucleus, the magnetoid, which gives rise to the characteristic non-thermal luminosity. The mass of the quasar is determined by its stars while the parameters of the magnetoid depend on the stage of evolution or conditions of formation in a similar way to those of radiogalaxies or active nuclei of galaxies.
In application/xml+jats
format
Archived Files and Locations
application/pdf
261.3 kB
file_ja747jv56vfcnbe5n6ncr5wnoi
| |
application/pdf
274.4 kB
file_7anif6d6tjcdvjmjfbccnfsqry
|
www.cambridge.org (web) web.archive.org (webarchive) |
access all versions, variants, and formats of this works (eg, pre-prints)
Crossref Metadata (via API)
Worldcat
SHERPA/RoMEO (journal policies)
wikidata.org
CORE.ac.uk
Semantic Scholar
Google Scholar