The equilibrium magnetized disks

Details The equilibrium magnetized disks The equilibrium magnetized disks

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.115..275b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 115, no. 2, Oct. 1985, p. 275-294.

Statistics

Computation

4

Computational Astrophysics, Equilibrium Equations, Gravitational Fields, Magnetic Fields, Spiral Galaxies, Unified Field Theory, Astronomical Models, Galactic Nuclei, Quasars

Scientific paper

In the present consideration of equilibrium figures in the form of thin rotating disks for modeling spiral galaxy flat components, analytical solutions are obtained for gravitational and magnetic fields at given distributions of area matter density and surface currents, and numerical solutions are obtained for a magnetized, nonrotating disk whose equilibrium is governed by the balance of magnetic and gravitational forces. The models are found to be unstable against short wave perturbations. Pressure, however, can contribute a few percent toward disk stabilization against such perturbations.

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