TY  - CONF
A1  - ud-Doula, A.
T1  - Large-scale wind structure due to magnetic fields
N2  - Magnetic fields influence the dynamics of hot-star winds and create large scale structure. Based on numerical magnetohydrodynamic (MHD) simulations, we model the wind of θ¹ Ori C, and then use the SEI method to compute synthetic line profiles for a range of viewing angles as function of rotational phase. The resulting dynamic spectrum for a moderately strong line shows a distinct modulation, but with a phase that seems at odds with available observations.
Y1  - 2008
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/1634
UR  - https://nbn-resolving.org/urn:nbn:de:kobv:517-opus-18010
ER  -