As part of a spectroscopic survey of emission-line objects in the Southern Hemisphere, we have observed and studied spectroscopically 33 objects from the list of Sanduleak & Stephenson (1973) (SS73 stars). We have proposed that 16 of them are Be stars, 5 are peculiar Be stars, 4 are T Tauri stars and 7 are M-type stars with emission lines and 1 Herbig object. The group named peculiar Be stars reveals more interesting features and they deserve further analysis based on high resolution spectra.
Acknowledgements
We thank Perry Berlind for having provide us with the spectra of VV Cep and DF Tau. We also thank D. F. Lopes, L. da Silva and S. L. Martins for having observed some stars in the present survey. C. S. Franco thanks CNPq for financial support.
Copyright ESO 2003