Large-scale wind structure due to magnetic fields
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 p...
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| Format: | Others |
| Language: | English |
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Universität Potsdam
2007
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| Online Access: | http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-18010 http://opus.kobv.de/ubp/volltexte/2008/1801/ |