Physics
Scientific paper
Jul 1971
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971phrvl..27..210d&link_type=abstract
Physical Review Letters, vol. 27, Issue 4, pp. 210-213
Physics
6
Scientific paper
The Goldreich-Schubert thermally driven turbulence extending to the deep interiors of solar-type stars which exhibit rotational slowing is precluded by spectroscopic observations showing the presence of lithium and beryllium. These observations, similar observations of the sun, the solar-wind torque, and the solar oblateness are consistent with a model for which such a turbulence is terminated at the surface of a rapidly rotating core containing 95% of the star's mass.
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