  We explore the dynamical behaviour of cosmological models involving a scalar
field (with an exponential potential and a canonical kinetic term) and a matter
fluid with spatial curvature included in the equations of motion. Using
appropriately defined parameters to describe the evolution of the scalar field
energy in this situation, we find that there are two extra fixed points that
are not present in the case without curvature. We also analyse the evolution of
the effective equation-of-state parameter for different initial values of the
curvature.
