Einstein's field equations for stationary Bianchi type II models with
a perfect fluid source are investigated. The field equations are rewri
tten as a system of autonomous first-order differential equations. Dim
ensionless variables are subsequently introduced for which the reduced
phase space is compact. The system is then studied qualitatively usin
g the theory of dynamical systems. It is shown that the locally rotati
onally symmetric models are not asymptotically self-similar for small
values of the independent variable. A new exact solution is also given
. (C) 1997 American Institute of Physics.