Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...505l..47c&link_type=abstract
Astrophysical Journal Letters v.505, p.L47
Astronomy and Astrophysics
Astronomy
8
Convection, Hydrodynamics, Stars: Evolution, Stars: Interiors, Stars: Rotation
Scientific paper
Shear-generated turbulent mixing in stellar radiative regions (stably stratified) has recently been found to be too weak. This has stimulated the search for the missing mixing. We suggest that there may not be a missing mixing problem. Phenomenological models have underestimated its real strength, thus leading to a negative assessment of its real potential.
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