  A set of equations of state obtained from finite-range Gogny forces and
momentum-dependent interactions is used to investigate the recent observation
of gravitational waves from the binary neutron star merger GW170817 event. For
this set of interactions, we have calculated the neutron star tidal
deformabilities (related to the second Love number), the mass-radius diagram,
and the moment of inertia~($I$). The $I$-Love relation has been verified. We
also have found strong correlations among the tidal deformability of the
canonical neutron star, its radius, and the derivatives of the nuclear symmetry
energy at the saturation density. Most of the obtained results are located
within the constraints of the tidal deformabilities extracted from the GW170817
detection.
