  We present the solution space of the field equations in the Einstein-aether
theory for the case of a vacuum Bianchi Type V space-time. We also find that
there are portions of the initial parameters space for which no solution is
admitted by the reduced equations. Whenever solutions do exist, their physical
interpretation is examined through the behavior of Ricci and/or Kretsmann
scalar, as well as with the identification of the effective energy momentum
tensor in terms of a perfect fluid. There are cases in which no singularities
appear and others where the effective fluid is isotropic.
