Orbital elements, which satisfy both positional measurements (visual a
nd interferometric) and also our radial velocity observations obtained
with a correlation spectrometer at favorable epochs when the lines of
the components were separated, have been found by a least squares met
hod for the visual binary stars BS 466=Kuiper 7 and ADS 16098. Values
have been determined for masses and orbital parallaxes. Their errors a
re calculated by considering the correlations of the errors for the in
dividual orbital elements, and the suitable equations are given.