96 faint classical Cepheids have been measured, each a small number of
times (4 to 7 times), in radial velocity, in order to calculate their
centre-of-mass radial velocity accurately enough for an analysis of t
he local galactic rotation. This paper contains the raw radial velocit
y data. The analysis and results are presented in a joint paper in the
Main Section of this journal (Pont et al. 1994).