No CrossRef data available.
Article contents
Hydrodynamical Models of Rotating Magnetic Winds
Published online by Cambridge University Press: 14 August 2015
Abstract
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
- Copyright
- Copyright © Reidel 1982