Differential rotation on the lower main
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M. KΓΌker; G. RΓΌdiger
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Article
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2005
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John Wiley and Sons
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English
β 412 KB
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## Abstract We compute the differential rotation of main sequence stars of the spectral types F, G, K, and M by solving the equation of motion and the equation of convective heat transport in a meanβfield formulation. For each spectral type the rotation rate is varied to study the dependence of the