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Explore a model for sOriE using RRM for photometry and Ha polarimetry observations to understand B-field tilt. Develop insights into the complex nature of stellar magnetic fields.
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RRM model for s Ori E B*~104 G h*~106 ! tilt ~ 55o
RRM model for s Ori E photometry EM +B-field B*~104 G => h*~106 ! tilt ~ 55o Ha polarimetry
Ha Observations s Ori E RRM Model