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Ultraviolet Line Profiles of Slowly Rotating Massive Star Winds Using the "analytic Dynamical Magnetosphere" Formalism

C. Erba,A. David-Uraz,V Petit,L. Hennicker,C. Fletcher,A. W. Fullerton,Y. Naze,J. Sundqvist,A. Ud-Doula

Monthly Notices of the Royal Astronomical Society（2021）

Cited 10|Views29
Key words
line: profiles,radiative transfer,stars: magnetic field,stars: massive,stars: winds,outflows,ultraviolet: stars
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