  We present exact solutions describing rotating, inhomogeneous dust with
generic initial data in 2+1 dimensional AdS spacetime and show how they are
smoothly matched to the Banados-Teitelboim-Zanelli (BTZ) solution in the
exterior. The metrics, which are the rotational analogues of the 2+1
dimensional LeMaitre-Tolman-Bondi (LTB) family, are described by their angular
momentum and one additional constant which, together with the angular momentum,
determines the energy density of the dust cloud. The weak energy condition
gives a constraint on the angular momentum profile inside the cloud. Solutions
can be stationary or time dependent, but only the time dependent solutions can
be matched consistently to a BTZ exterior. No singularity is formed in either
the stationary or the time dependent cases.
