  We present exact solutions in Einstein-aether theory in a static spherically
symmetric background space with a spacelike aether field, as a difference with
the usual selection of timelike aether field. We assume a coupling between the
scalar field and the aether field introduced in the aether coefficients. The
exact spacetimes describe hairy black hole solutions for which the limits of
the Schwarzschild, de-Sitter Schwarzschild and Reissner-Nordstr\"om metrics are
recovered.
