One of the strongest evidences of the AdS/CFT correspondence is provided by three-dimensional gravity with a negative cosmological constant, whose asymptotic symmetry group is the conformal one. As a further example, one can consider gravity coupled to self-interacting scalar field having a slow fall-off at infinity. In these cases, the metric describes an asymptotically AdS spacetime in a relaxed sense as compared with the one of Brown and Henneaux. Nevertheless, the asymptotic symmetry group remains to be the same as in pure gravity. In this talk we show a wide class of scalar hairy black holes, including spinning ones, which fit in these asymptotic conditions.