  We obtain rotation laws for axially symmetric, selfgravitating and stationary
fluids around spinning black holes. They reduce --- in the Newtonian limit ---
to monomial rotation curves. For spinless black hole, one obtains in the first
post-Newtonian (1PN) approximation the hitherto known results, that can be
interpreted as the geometric dragging and material antidragging. We find new
1PN effects, that are due to spins of black holes.
