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Wind-Compressed Disks
Published online by Cambridge University Press: 12 April 2016
Abstract
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
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- Copyright © Springer-Verlag 1999
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