  We consider tachyonic warm-inflationary models in the context of intermediate
inflation. We derive the characteristics of this model in slow-roll
approximation and develop our model in two cases, 1- For a constant dissipative
parameter $\Gamma$. 2- $\Gamma$ as a function of tachyon field $\phi$. We also
describe scalar and tensor perturbations for this scenario. The parameters
appearing in our model are constrained by recent observational data. We find
that the level of non-Gaussianity for this model is comparable with
non-tachyonic model.
