Back to the Abstract

	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
	References

	List of tables
	List of figures