  We present the first results of a campaign to obtain orbital solutions of
subdwarf B (sdB) stars from the Edinburgh-Cape survey. We have obtained blue
spectra of 35 sdBs, 20 of which have been observed in more than two epochs. 15
out of the 35 are certain binaries with a few other objects showing radial
velocity variations with small amplitude, possibly long period sdB binaries. We
have secured the orbital parameters for 2 of the 15 systems and narrowed down
the orbits of another one to a small range of periods. These preliminary
results only use data taken up to December 2003.
