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Nonradiative Heating and Enhanced Mass-loss Due to Shear Turbulence in Massive Hot StarsRotation in massive stars generates shear turbulence. This has the consequence of heating the outer layers of massive stars and enhancing mass-loss in the early spectral types. Model calculations are presented and discussed in support of these effects.
Document ID
19850009471
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Sreenivasan, S. R. (Calgary Univ. Alberta)
Wilson, W. J. F. (Calgary Univ. Alberta)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: NASA. Goddard Space Flight Center The Origin of Nonradiative Heating(Momentum in Hot Stars
Subject Category
Astrophysics
Accession Number
85N17780
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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