Stochastic model of fragmented structures in galaxies

Details Stochastic model of fragmented structures in galaxies Stochastic model of fragmented structures in galaxies

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..897r&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Sept.-Oct. 1991, p. 897-908. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Galactic Structure, Stochastic Processes, Density Distribution, Gravitational Fields, Mathematical Models, Rotating Disks

Scientific paper

An inhomogeneous stationary rotating disk is considered. The medium is assumed to have negligible pressure. It is shown that the ensemble of the density inhomogeneities is a mixing system. The space structure of a collective gravitational field of density inhomogeneities is analyzed, and this field is found to have a large-scale spiral structure. The density inhomogeneities are distributed on a disk in accordance with this structure, whose fractal dimension depends on the number of inhomogeneities.

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