  We perform dynamical analysis of anisotropic Rastall cosmologies and, in
particular Kantowski-Sachs, locally rotationally symmetric (LRS) Bianchi I and
LRS Bianchi III cosmologies. Using dynamical system techniques, a qualitative
analysis of cosmological equations yield physically interesting cases which are
in agreement with observations such as de Sitter, accelerating, stable
attractors are isotropic. Features such as isotropization and cosmological
bounce are discussed in detail.
