Nonradiative heating and enhanced mass-loss due to shear turbulence in massive hot stars

Details Nonradiative heating and enhanced mass-loss due to shear turbulence in massive hot stars Nonradiative heating and enhanced mass-loss due to shear turbulence in massive hot stars

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..177s&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 177-182 (SEE N85-17755 08-88)

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Computation

Heating, Hot Stars, Stellar Mass Ejection, Stellar Rotation, Stellar Winds, Turbulence, Computation, Computer Programs, Ions, Mathematical Models, Nitrogen, Oxygen, Stellar Models, Stellar Structure

Scientific paper

Rotation 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.

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