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• W2086249938 abstract "Context. The presence of magnetic fields in O-type stars has been suspected for a long time. The discovery of these fields would explain a wide range of well documented enigmatic phenomena in massive stars, in particular cyclical wind variability, Hα emission variations, chemical peculiarity, narrow X-ray emission lines, and non-thermal radio/X-ray emission." @default.
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• W2086249938 date "2008-09-11" @default.
• W2086249938 modified "2023-10-17" @default.
• W2086249938 title "Magnetic field measurements of O stars with FORS 1 at the VLT" @default.
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• W2086249938 doi "https://doi.org/10.1051/0004-6361:200810171" @default.
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