Abstract:
Spectra of MV Sgr obtained at CTIO in 1992 May show many emission lines in the red. Most of the emission lines show two components with a minimum centred at the stellar velocity. Species represented include H, HeI, TiII and FeII. Of special interest is emission in the LiI 6707-A resonance doublet. [OI] and [NII] emission indicate the presence of a nebula around the star. The radial velocity of the absorption lines (AlIII, SiIII, NII and CII) and FeII emission lines agrees with the radial velocity given by Jeffery et al.
