Physics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.289..569l&link_type=abstract
Nature, vol. 289, Feb. 12, 1981, p. 569, 570.
Physics
1
Magnetic Stars, Star Clusters, Stellar Rotation, Supermassive Stars, Active Galactic Nuclei, Gravitational Collapse, Life (Durability), Quasars, Seyfert Galaxies, Stellar Envelopes, Stellar Luminosity, Stellar Mass, Stellar Mass Accretion, Stellar Radiation, Velocity Distribution
Scientific paper
The disruption of the main body of a nuclear magnetoid and the formation of a dense core subject to explosion and/or gravitational collapse are shown to be the results of the interaction of a magnetoid and a star cluster. It is assumed that the star cluster has an isotropic velocity distribution. It is concluded that a magnetoid formed in an ordinary galactic nucleus will be disrupted in approximately 10,000 years to leave a dense star cluster surrounding a black hole. The black hole will be able to power an active galactic nucleus for the period greater than a million years required to explain the activity of Seyfert galaxies and quasars.
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