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Paper: |
A Rigidly Rotating Magnetosphere Model for the Circumstellar Environments of Magnetic OB Stars |
Volume: |
337, The Nature and Evolution of Disks Around Hot Stars |
Page: |
314 |
Authors: |
Townsend, R.; Owocki, S.; Groote, D. |
Abstract: |
We report on a new model for the circumstellar environments of rotating, magnetic hot stars. This model predicts the channeling of wind plasma into a corotating magnetosphere, where — supported against gravity by centrifugal forces — it can steadily accumulate over time. We apply the model to the B2p star σ Ori E, demonstrating that it can simultaneously reproduce the spectroscopic, photometric and magnetic variations exhibited by the star. |
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