We report 490 radial velocities for 16 Galactic Cepheid variables. The typical uncertainty of a single velocity is ±0.40 km s -1 . Comparison with published velocities shows excellent agreement. Two of the Cepheids (Z Lac, S Sge) are known binaries and exhibit orbital velocity changes in our observing interval.
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Barnes et al. (2005) studied this question.
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