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Article Contents
1 Introduction
2 Conservation of angular momentum in 2 dimensional hydrodynamical algorithms
3 Coupling of the 2D grid with a 1D grid
4 Performance of the code
5 Astrophysical applications
6 Conclusion and perspectives
Appendix A: Open boundary condition
Appendix B: Benchmarking

List of tables
List of figures

Copyright ESO 2007
Published by EDP Sciences