Models of self-gravitating accretion disks

Details Models of self-gravitating accretion disks Models of self-gravitating accretion disks

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253..318b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 1, Jan. 1992, p. 318-328.

Astronomy and Astrophysics

Astrophysics

14

Accretion Disks, Active Galactic Nuclei, Gravitational Fields, Density Distribution, Gray Scale, Iterative Solution, Poisson Equation

Scientific paper

An iterative procedure which produces a final density distribution in equilibrium with the potential generated by it is presently used to compute the equilibrium structure of a self-gravitating thick accretion disk. Attention is given to the primary differences among the properties of the models thus computed with those derived from models computed in the absence of self-gravitation.

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