|
![Back to Volume](/images/back_to_volume.png) |
Paper: |
σ Ori E: The Archetypal Rigidly Rotating Magnetosphere |
Volume: |
361, Active OB-Stars: Laboratories For Stellar and Circumstellar Physics |
Page: |
110 |
Authors: |
Townsend, R.H.D. |
Abstract: |
I review the basic concepts of the Rigidly Rotating Magnetosphere model for the circumstellar plasma distribution around the helium-strong star σ Ori E. I demonstrate that the model can furnish a good fit to the photometric, spectroscopic and magnetic variability exhibited by this star, and argue that the variability of other helium-strong stars may be amenable to a similar interpretation. |
|
![Back to Volume](/images/back_to_volume.png) |
|
|