Physics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..142f&link_type=abstract
In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 142-147 (SEE N85-17755 08-88)
Physics
Angular Momentum, Hot Stars, Magnetic Fields, Rotating Fluids, Stellar Rotation, Stellar Winds, Equations Of Motion, Luminosity, Mass Transfer, Radiation Pressure, Stellar Mass, Terminal Velocity
Scientific paper
The 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.
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