Formation of disks around hot magnetic stars under the action of radiation pressure

Details Formation of disks around hot magnetic stars under the action of radiation pressure Formation of disks around hot magnetic stars under the action of radiation pressure

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pazh...16.1030b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 16, Nov. 1990, p. 1030-1044. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

3

Hot Stars, Magnetic Stars, Radiation Pressure, Space Plasmas, Magnetohydrodynamic Flow, Plasma Diffusion, Plasma Jets, Supersonic Flow

Scientific paper

A model of a plasma envelope of an isolated hot magnetic star with high radiation pressure directed from the surface is considered. The characteristics of an equatorial plasma disk formed under the action of the radiation pressure are defined for various mass loss rates from the star surface. The conditions of the disk stability are analyzed. Subsonic and supersonic stationary plasma flows from the star surface to the disk are studied, as well as radial diffusion of substance to the disk periphery.

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