Structure of neutron stars with unified equations of state

We present a set of three unified equations of states (EoSs) ba sed on the nuclear energy-density functional (EDF) theory. These EoSs are based on generalized Skyrme forces fitted to essentially all experimental atomic mass data and constrained to reproduce various properties of infinite nuclear matter as o btained from many-body cal- culations using realistic two- and three-body interaction s. The structure of cold isolated neutron stars is discussed in connection with some astrophysical observations.