Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22..473k&link_type=abstract
(Astrofizika, vol. 22, May-June 1985, p. 473-485) Astrophysics (ISSN 0571-7132), vol. 22, no. 3, Nov. 1985, p. 280-288. Translat
Astronomy and Astrophysics
Astrophysics
Astronomical Models, Cosmic Plasma, Galactic Clusters, Ion Density (Concentration), Plasma Composition, Self Consistent Fields, Boundary Value Problems, Gravitational Fields
Scientific paper
A self-consistent model for determining the state of the plasma component in a galactic cluster is developed. It is shown that deriving the distribution of the hydrodynamic parameters of a cluster using the polytropic equation of state reduces in the last analysis to solving the boundary-value problem for the gravitational potential of a self-consistent field. The model for the plasma component in this case is determined by three main parameters. Equations are obtained which determine the distribution of ions throughout a cluster plasma under conditions of ion diffusion equilibrium. The main types of solution are found for the plasma component, and an algorithm is constructed in order to solve the problem with an allowance for the ion composition of the plasma.
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