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Here I present first results from the ESO-VLT Multi-Instrument Kinematic Survey of Galactic Globular Clusters, a survey specifically designed to provide line-of-sight velocities of hundreds individual stars over the entire radial extension of a selected sample of globulars. The survey allows the first kinematical exploration of the innermost regions of high- density clusters. Moreover, once combined with proper motion measurements (from multi-epoch HST observations and from Gaia), it willdoi:10.5281/zenodo.2595129 fatcat:6iz73i42nnawlicbhaoir3rrcm