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Article Contents
1 Introduction
2 Selection procedure
3 Data reduction
4 $\mathsf{E(V-L)}$, polarization and v sin i as a function of spectral type
5 Distributions of projected rotational velocities
6 Distributions of near and far IR excesses
7 Distributions of intrinsic polarization for different subgroups of Be stars
8 Discussion
9 Conclusions
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Copyright ESO 2001
Published by EDP Sciences