New aspects in the theory of magnetic winds from massive hot stars

Details New aspects in the theory of magnetic winds from massive hot stars New aspects in the theory of magnetic winds from massive hot stars

1998-04-16

arxiv.org/abs/astro-ph/9804152v1

Astronomy and Astrophysics

Astrophysics

PhD thesis accepted by the university of Bonn. 79 pages with 31 Postscript figures using LaTeX2e with rotating,epsfig, amssymb

Scientific paper

This thesis discusses the influence of magnetic fields on the instability of line-driven winds in O-stars and Wolf-Rayet stars. This combination is an important concept to understand the strong, observed winds from Wolf-Rayet stars. In the second part of the thesis a model is derived which describes the wind outside the equatorial plane. This model allows to use the simple approach of an ordinary differential equation instead of a 2-dim. partial differential equation.

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