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- W2328519260 abstract "Abstract As per the recent study by the MiMeS collaboration, only about 10% of massive stars possess organized global magnetic fields, typically dipolar in nature. The competition between such magnetic fields and highly non-linear radiative forces that drive the stellar winds leads to a highly complex interaction. Such an interplay can lead to a number of observable phenomena, e.g. X-ray, wind confinement, rapid stellar spindown. However, due to its complexity, such an interaction cannot usually be modeled analytically, instead numerical modeling becomes a necessary tool. In this talk, I will discuss how numerical magnetohydrodynamic (MHD) simulations are employed to understand the nature of such magnetized massive star winds." @default.
- W2328519260 created "2016-06-24" @default.
- W2328519260 creator A5076607230 @default.
- W2328519260 date "2014-06-01" @default.
- W2328519260 modified "2023-09-25" @default.
- W2328519260 title "Magnetic Field - Stellar Winds Interaction" @default.
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- W2328519260 doi "https://doi.org/10.1017/s1743921314007029" @default.
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