  We consider an Einstein-aether scalar field cosmological model where the
aether and the scalar field are interacting. The model of our consideration
consists the two different interacting models proposed in the literature by
Kanno et al. and by Donnelly et al. We perform an extended analysis for the
cosmological evolution as it is provided by the field equations by using
methods from dynamical systems; specifically, we determine the stationary
points and we perform the stability analysis of those exact solutions.
