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Article Contents
1 Introduction
2 The winds of B[e] supergiants
3 The wind model
4 Ionization radii in a wind with non-spherical density distribution
5 Ionization structure of H and He
6 Discussion
7 Comparison with observations from other hot stars
8 Conclusion
Appendix A: Derivation of the classical Strömgren sphere

List of tables
List of figures

Copyright ESO 2003
Published by EDP Sciences