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Winds from Rotating, Magnetic, Hot StarsThe effect of a magnetic field coupled with stellar rotation on the wind from a hot star, which is driven primarily by line radiation pressure, is discussed.
Document ID
19850009466
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Friend, D. B. (National Center for Atmospheric Research Boulder, CO, United States)
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
85N17775
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19850009446Collected WorksThe Origin of Nonradiative Heating/momentum in Hot Stars
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