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Hydrodynamical Models of Rotating Magnetic Winds

Published online by Cambridge University Press:  14 August 2015

Paul K. Barker
Paul K. Barker*
Affiliation:
The University of Western Ontario

Abstract

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Numerical investigations of rotating stellar winds driven by a combination of magnetic and line radiation forces show a clear dichotomy: shallow winds have their azimuthal velocity enhanced by magnetic corotation, whereas steep winds may have a diminished circular velocity.

Type
VIII. Atmospheric Models
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 485 - 488
Copyright
Copyright © Reidel 1982 

References

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