Quasar evolution and gravitational collapse

Details Quasar evolution and gravitational collapse Quasar evolution and gravitational collapse

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...269...57c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 269, June 1, 1983, p. 57-72. Research supported by the Consiglio Nazionale

Astronomy and Astrophysics

Astronomy

33

Galactic Nuclei, Gravitational Collapse, Quasars, Radio Galaxies, Astronomical Models, Black Holes (Astronomy), Evolution (Development), Luminosity, Mass Flow, Rotating Bodies

Scientific paper

The role of gravity is considered along with the modes of energy release. A description of a general statistical framework is presented, taking into account two extreme cases. The modes of evolution are discussed, and the basic solutions are examined in some details. Attention is given to the brightening phase and rarefaction, the brightening phase and condensation, the dimming phase, and the case in which brightening and dimming are coupled. Models describing the release of gravitational energy are also investigated, taking into consideration accretion onto a black hole, rotating magnetized configurations, and accretion flows onto magnetized rotators.

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