Statistics – Applications
Scientific paper
May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.7110m&link_type=abstract
American Astronomical Society, 188th AAS Meeting, #71.10; Bulletin of the American Astronomical Society, Vol. 28, p.943
Statistics
Applications
Scientific paper
The possible existence of stagnation zones in the atmospheres of hot stars with rotation and magnetic fields is considered. Solutions of the structure equations for atmospheres in axially symmetric stars are obtained. Gravity, centrifugal force, lorentz force and forces due to radiation are included in the models considered. The solutions that are obtained in this study require the presence of a nonzero transverse component of the magnetic field at the equator. It is also found that magnetic fields that are purely radial in the equatorial region cannot help maintain stagnation zones in such a region. Results for some of the cases studied are presented. These results may have useful applications in the study of wind compressed disks.
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