Physics
Scientific paper
Mar 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..110t&link_type=abstract
Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere
Physics
Scientific paper
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.
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