We present the results of an interferometric study of the N2H + (1–0) emission from nine nearby, isolated, low-mass protostellar cores, using the OVRO millimeter array. The main goal of this study is the kinematic characterization of the cores in terms of rotation, turbulence, and fragmentation. Eight of the nine objects have compact N2H + cores with FWHM radii of 1200 − 3500 AU, spatially coin...