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• W2032933678 abstract "Context. Oblique magnetic dipole fields have been detected in Bp stars for several decades, and more recently also in normal massive stars. In the past decade, it has been established that stellar magnetospheres form through the channelling and confinement of an outflowing stellar wind by the stellar magnetic field. This explains specific properties of magnetic massive stars, such as their rotationally modulated photometric light curve, Hα emission, UV spectra, and X-ray emission." @default.
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• W2032933678 date "2012-10-01" @default.
• W2032933678 modified "2023-10-15" @default.
• W2032933678 title "HD 96446: a puzzle for current models of magnetospheres?" @default.
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• W2032933678 doi "https://doi.org/10.1051/0004-6361/201218988" @default.
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