We have obtained velocities for the binary Cepheid V350 Sgr at the Dav
id Dunlap Observatory. An orbit has been derived combining these data
with velocities from the literature. The spectral type of B9.0 V has b
een confirmed from an IUE spectrum, leading to a mass of the companion
of 2.5 M.. The uncertainty in the mass is also discussed. (C) 1997 Am
erican Astronomical Society.