Magnetic Models of Circumstellar Clouds around Massive Stars

Details Magnetic Models of Circumstellar Clouds around Massive Stars Magnetic Models of Circumstellar Clouds around Massive Stars

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..33...80o&link_type=abstract

Massive Stars: Fundamental Parameters and Circumstellar Interactions (Eds. P. Benaglia, G. L. Bosch, & C. E. Cappa) Revista Mexi

Astronomy and Astrophysics

Astronomy

Stars: Mass Loss, Stars: Magnetic Fields, Magnetohydrodynamics

Scientific paper

This talk reviewed recent efforts to develop dynamical models for the effects of a surface dipole field on radiatively driven wind outflows. One particular project applies magnetohydrodynamic (MHD) simulations of a Magnetically Confined Wind Shock (MCWS) model (originally developed by Babel & Montmerle 1997) to explain X-ray emission observed by Rosat (Gagné et al. 1997) from the magnetic O7V star θ^{1 Ori C.

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