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Article Contents
1 Introduction
2 Targets and scope of the investigation
3 Spectropolarimetric observations
4 Field modelling procedure and input physics
5 $\vec\beta$ Coronae Borealis
6 53 Camelopardalis
7 Comments on the element abundance distributions
8 Reliability of stellar magnetic field models
9 Conclusions

Copyright ESO 2001
Published by EDP Sciences