Radial velocities have been determined for a sample of 2930 B2-F5 stars, 95
% observed by the Hipparcos satellite in the north hemisphere and 80% witho
ut reliable radial velocity up to now. Observations were obtained at the Ob
servatoire de Haute Provence with a dispersion of 80 Angstrom mm(-1) with t
he aim of studying stellar and galactic dynamics. Radial velocities have be
en measured by correlation with templates of the same spectral class. The m
ean obtained precision is 3.0 km s(-1) with three observations. A new MK sp
ectral classification is estimated for all stars.