Back to the Abstract

	1 Introduction
	2 AMBER/VLTI observations
	3 Reduction of the interferometric data
	4 Study of the envelope morphology using simple models
	5 The SIMECA code: a brief description
	6 Using SIMECA for the modeling of Arae circumstellar environment
	7 Discussion
	8 Conclusion
	References

	List of tables
	List of figures