Impact of non-uniform surface magnetic fields on stellar winds
نویسندگان
چکیده
منابع مشابه
Impact of non-uniform surface magnetic fields on stellar winds
Observations of active stars reveal highly non-uniform surface distributions of magnetic flux. Theoretical models considering magnetised stellar winds however often presume uniform surface magnetic fields, characterised by a single magnetic field strength. The present work investigates the impact of non-uniform surface magnetic field distributions on the stellar mass and angular momentum loss r...
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Hirotaka Ito,1 Shoichi Yamada,1 Kohsuke Sumiyoshi,2 and Shigehiro Nagataki3 1Department of Physics, Science, and Engineering, Waseda University, Okubo, 3-4-1, Shinjuku, Tokyo 169-8555, Japan & Advanced Research Institute for Science and Engineering, Waseda University, Okubo, Shinjuku, Tokyo 169-8555, Japan 2Numazu College of Technology, Ooka 3600, Numazu, Shizuoka 410-8501, Japan & Division of ...
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ژورنال
عنوان ژورنال: Astronomy & Astrophysics
سال: 2005
ISSN: 0004-6361,1432-0746
DOI: 10.1051/0004-6361:20053110