1 INTRODUCTION

2 OBSERVATIONS

3 SPECTRAL CLASSIFICATION

4 STELLAR PARAMETERS FROM PHOTOMETRY AND SED
4.1 Photometric parameters
4.2 Effective Temperature from SED

5 SPECTROSCOPIC ANALYSIS
5.1 Analysis of hydrogen lines
5.2 Atmospheric parameters from iron lines analysis
5.3 Abundances analysis
5.4 Discussion of the results

6 DISCUSSION AND CONCLUSIONS