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- W1748659860 abstract "Since 2002, strong, organized magnetic fields have been firmly detected at the surfaces of about 10 Galactic O-type stars. In this paper I will review the characteristics of the inferred fields of individual stars, as well as the overall population. I will discuss the extension of the 'magnetic desert', first inferred among the A-type stars, to O stars up to 60 solar masses. I will discuss the interaction of the winds of the magnetic stars with the fields above their surfaces, generating complex 'dynamical magnetosphere' structures detected in optical and UV lines, and in X-ray lines and continuum. Finally, I will discuss the detection of a small number of variable O stars in the LMC and SMC that exhibit spectral characteristics analogous to the known Galactic magnetic stars, and that almost certainly represent the first known examples of extra-Galactic magnetic stars." @default.
- W1748659860 created "2016-06-24" @default.
- W1748659860 creator A5005424993 @default.
- W1748659860 date "2014-11-13" @default.
- W1748659860 modified "2023-09-27" @default.
- W1748659860 title "Review: Magnetic fields of O stars" @default.
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- W1748659860 hasPublicationYear "2014" @default.
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