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[en] The authors present some examples where the physics of stellar rotation is not completely clear. Three questions are considered: a) Can the angular velocity vary on equipotential surfaces; b) What is the time scale of Goldreich-Schubert-Fricke instabilities; and c) How fast is circulation in surface-near regions. (Auth.)
Source
Sugimoto, D. (Tokyo Univ. (Japan)); Lamb, D.Q. (Harvard Univ., Cambridge, MA (USA). Center for Astrophysics); Schramm, D.N. (Chicago Univ., IL (USA)) (eds.); International Astronomical Union; 362 p; ISBN 90-277-1274-3; 
; 1981; p. 237-256; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 93 on fundamental problems in the theory of stellar evolution; Kyoto, Japan; 22 - 25 Jul 1980
; 1981; p. 237-256; D. Reidel; Dordrecht, Netherlands; International Astronomical Union symposium no. 93 on fundamental problems in the theory of stellar evolution; Kyoto, Japan; 22 - 25 Jul 1980