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Wind-Compressed Disks

Published online by Cambridge University Press:  12 April 2016

Jon E. Bjorkman*
Affiliation:
University of Toledo, Dept. of Physics and Astronomy, Toledo, OH 43606, USA

Abstract

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We discuss the wind-compressed disk (WCD) model and its ability to produce disks in the outflows from rapidly rotating stars. In particular, we discuss the recently discovered non-radial force components that may inhibit the formation of the disk and present preliminary investigations of the ionization distribution and associated line profiles in the WCD model.

Type
Section II Theory of Non-spherical Winds
Copyright
Copyright © Springer-Verlag 1999

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