Spectroscopic binary orbits from ultraviolet radial velocities. Paper 31: Stars with few IUE observations

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Scientific paper

All O-type stars known to be or suspected of being binary, and which
have short-wavelength high-resolution IUE observations, but which have
not yet been dealt with in the present series, have been examined for
velocity variability, in both the UV and optical. Several new orbital
solutions are suggested.

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