  Warm-intermediate inflationary universe models in the context of braneworld
cosmologies, are studied. This study is done in the weak and strong dissipative
regimes. We find that, the scalar potentials and dissipation coefficients in
terms of the scalar field, evolves as type-power-law and powers of logarithms,
respectively. General conditions required for these models to be realizable are
derived and discussed. We also study the scalar and tensor perturbations for
each regime. We use recent astronomical observations to constraint the
parameters appearing in the braneworld models.
