We use two models for the distribution function to solve an inverse pr
oblem for axisymmetric disks. These systems may be considered - under
certain assumptions - as galactic disks. In some cases the solutions o
f the resulting integral equations are simple, which allows the determ
ination of the kinematic properties of self-consistent models for thes
e systems. These properties for the n = 1 Toomre disk are presented in
this study.