  We find solutions for quantum Class A Bianchi models of the form $\rm \Psi=W
e^{\pm \Phi}$ generalizing the results obtained by Moncrief and Ryan in
standard quantum cosmology. For the II and IX Bianchi models there are other
solutions $\rm \tilde\Phi_2$, $\rm \tilde\Phi_9$ to the Hamilton-Jacobi
equation for which $\rm \Psi$ is necessarely zero, in contrast with solutions
found in supersymmetric quantum cosmology.
