  We study homogeneous and isotropic cosmologies in a Weyl spacetime. We show
that for homogeneous and isotropic spacetimes, the field equations can be
reduced to the Einstein equations with a two-fluid source. We write the
equations as a two-dimensional dynamical system and analyze the qualitative,
asymptotic behavior of the models. We examine the possibility that in certain
theories the Weyl 1-form may give rise to a late accelerated expansion of the
Universe and conclude that such behaviour is not met as a generic feature of
the simplest cosmologies.
