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Article Contents
1 Introduction
2 SIMECA: A code dedicated to active hot stars
3 The particular case of $\gamma $ Cas
4 Effect of the wind density
5 Effect of the effective temperature
6 Effect of the spectral type
7 Effect of the geometrical thickness of the disk
8 Effect of the inclination angle
9 Effect of rotational and terminal wind velocity
10 Conclusion and discussion
References

Copyright ESO 2001
Published by EDP Sciences