  In this paper, we discuss the dynamics of two- scalar-field cosmological
models. Unlike in the situation of exponential potential, we find that there
are late-time attractors in which one scalar field dominates the energy density
of universe and the other one decay. We also discuss the possibility of
multiple attractors model which is useful to realize the evolution of the
universe from a scaling era to recent acceleration era. We also give the
conditions of the existence of multiple attractors.
