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Article Contents
1 Introduction
2 Observations and data reduction
3 Orbital solution
4 Spectral type determination
5 The emission lines and Doppler tomography
6 The absorption lines and the Struve-Sahade effect
7 Modeling the spectra with an atmosphere code
8 The evolutionary status of HD 47 129
9 Conclusion

List of tables
List of figures

Copyright ESO 2008
Published by EDP Sciences