A nonrotating magnetized disk in equilibrium - The plane analog of the N = 3 polytrope

Details A nonrotating magnetized disk in equilibrium - The plane analog of the N = 3 polytrope A nonrotating magnetized disk in equilibrium - The plane analog of the N = 3 polytrope

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..395b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, May 1985, p. 395-399) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Equilibrium Equations, Gravitational Fields, Magnetic Fields, Polytropic Processes, Rotating Disks, Galactic Nuclei, Quasars

Scientific paper

Numerical models are constructed for a magnetized but nonrotating disk
kept in equilibrium by the balance between magnetic and gravitational
forces. The solutions are unstable against disturbances of short
wavelength, unless a small pressure term is introduced.

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