Casamiquela, L.L.CasamiquelaCarrera, R.R.CarreraJordi, C.C.JordiPancino, ElenaElenaPancino2020-09-172020-09-172016-05-01https://hdl.handle.net/20.500.13025/5023VizieR On-line Data Catalog J/MNRAS/458/3150. Originally published in 2016MNRAS.458.3150CWe present results of radial velocities for stars in 12 completed clusters (77 stars), and the reference stars Arcturus and mu Leo. This is a total of 79 stars. We include radial velocities from individual spectra, and final radial velocities from combined spectra which reach a minimum signal-to-noise ratio of 70. Comparison with the literature is included in the cases which the stars had previous measurements. (2 data files).Milky WayClusters openRadial velocities Comment table5.dat 401x64 *Radial velocities from individual spectra; table6.dat 78x348 *Final radial velocities and literature comparisonhttp://adsabs.harvard.edu/abs/2016yCat..74583150C2016yCat..74583150C