The shape of dense structures in plasma envelopes of slowly rotating stars

Details The shape of dense structures in plasma envelopes of slowly rotating stars The shape of dense structures in plasma envelopes of slowly rotating stars

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pazh...17..810b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 17, Sept. 1991, p. 810-816. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Dense Plasmas, Hot Stars, Magnetic Stars, Magnetohydrodynamic Stability, Stellar Rotation, Magnetic Dipoles, Radiation Pressure, Stellar Envelopes

Scientific paper

A geometric structure of the dense formations in the plasma envelopes of rotating hot magnetic stars whose radiation pressure force on plasma exceeds the gravity force is found. Problems of the stability of dense plasma structures are investigated. The influence of rotation effects on electromagnetic radiation of the plasma envelopes considered is discussed.

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