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Article Contents
1 Introduction - Motivation
2 Main assumptions
3 Transport of angular momentum
4 Transport of chemicals
5 Structural properties of the differentially rotating star
6 Thermal imbalance and transport of heat
7 Boundary conditions
8 Conclusion
Online Material
Appendix A: Algebra related to the spherical harmonics
Appendix B: System of transport equations for l = 2, 4

Copyright ESO 2004
Published by EDP Sciences