Back to the Abstract

	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
	References

	List of tables
	List of figures