THE EMISSION-LINE SPECTRUM OF THE HOT R-CORONAE-BOREALIS STAR MV SGR

Spectra of MV Sgr obtained at CTIO in 1992 May show many emission line s in the red. Most of the emission lines show two components with a mi nimum centred at the stellar velocity. Species represented include H, He I, Ti II and Fe II. Of special interest is emission in the Li I 670 7-Angstrom resonance doublet. [O I] and [N II] emission indicate the p resence of a nebula around the star. The radial velocity of the absorp tion lines (Al III, Si III, N II and C II) and Fe II emission lines ag rees with the radial velocity given by Jeffery et al.