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Article Contents
1 Introduction
2 Program stars and observational material
3 Methods of analysis
4 Abundance results
5 Discussion
6 Conclusion
References
Online Material
Appendix A: Examples of comparison between observed and synthetic Ne line profiles
Appendix B: log gf values, EW measurements and line-by-line abundances

List of tables
List of figures

Copyright ESO 2008
Published by EDP Sciences