Physics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..199u&link_type=abstract
In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 199-220 (SEE N85-17755 08-88)
Physics
Heating, Hot Stars, Magnetohydrodynamic Flow, Stellar Atmospheres, Stellar Magnetic Fields, Binary Stars, Comparison, Early Stars, Emission, Late Stars, Momentum, Stellar Coronas, Stellar Temperature, Sun, X Rays
Scientific paper
Possible magnetic effects in the heating and modification of flows in early type star atmospheres are discussed by referring to the physically related phenomena dealt with for late type stars, young stars, and close binary systems. It is pointed out as the result of that the magnetic field may play important roles also in early type star atmospheres in converting the energy of the radiatively driven outflow into heat, or in modifying the outflow by nozzling or by initial modification of temperature and/or momentum by which the effect of the radiation pressure may be made the most of in accelerating the outflow.
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