Non-radiative energy from differential rotation in hot stars

Details Non-radiative energy from differential rotation in hot stars Non-radiative energy from differential rotation in hot stars

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..164c&link_type=abstract

In its The Origin of Nonradiative Heating/Momentum in Hot Stars p 164-168 (SEE N85-17755 08-88)

Physics

1

Heating, Hot Stars, Luminosity, Spherical Harmonics, Stellar Coronas, Stellar Rotation, X Rays, Fluid Flow, Gravitational Effects, Magnetic Fields, Navier-Stokes Equation, Thermal Energy

Scientific paper

A model of differential rotation is proposed for the upper radiative
envelopes of hot stars, and it is suggested that the actions of such
motions can be the source of energy for heating the coronae.

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