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Article Contents
1 Introduction
2 Rotational perturbation of magneto-acoustic oscillations
3 A single mode seen as a multiplet in the observer's system
4 Application to $\ell ={1}$
5 Application to a representative model of roAp star
6 Conclusion and discussion
7 The $C_{\vec{n}\ell}$ and $D_{\vec{n}\ell}$ coefficients
References

Copyright ESO 2002
Published by EDP Sciences