ON THE DYNAMICS OF RADIATIVE ZONES IN ROTATING STARS

Abstract. In this lecture I try to explain the basic dynamical processes at work in a radiative zone of a rotating star. In particular, the no-tion of baroclinicity is thoroughtly discussed. Attention is specially directed to the case of circulations and the key role of angular momen-tum conservation is stressed. The specic part played by viscosity is also explained. The old approach of Eddington and Sweet is reviewed and criticized in the light of the seminal papers of Busse 1981 and Zahn 1992. Other examples taken in the recent literature are also presented; nally, I summarize the important points.