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Article Contents
1 Introduction
2 The spectrum of Hu 1-2
3 Chemical composition of the nebula
4 Comparison with other abundance determinations
5 The central star
6 Recombination line radiation
7 Discussion
8 Summary and conclusion
Appendix A: Visual lines
Appendix B: Ultraviolet (IUE) lines
References

Copyright ESO 2003
Published by EDP Sciences