  In this paper we introduce the "warm vector inflation" scenario. In warm
inflation scenario radiation is produced during the inflation epoch and
reheating is avoided. Slow-roll and perturbation parameters of this model are
presented. We develop our model using intermediate inflation model. In this
case, the model is compatible with observational data. We also study the model
using another exact cosmological solution, named logamediate scenario. We
present slow-roll and Hubble parameters, power spectrum and tensor-scalar ratio
in terms of inflaton. The model is compatible with WMAP7 and Planck
observational data.
