  Non-abelian gauge field inflation is studied in the context of warm inflation
scenario. We introduce this scenario as a mechanism that gives an end for
gauge-flation model. Slow-roll parameters and perturbation parameters are
presented for this model. We find the general conditions which are required for
this model to be realizable in slow-roll approximation. We also develop our
model in the context of intermediate and logamediate scenarios which are exact
solutions of inflationary field equation in the Einstein theory. General
expressions of slow-roll parameters, tensor-scalar ratio and scalar spectral
index are presented in terms of inflaton field for these two cases. Our model
is compatible with recent observational data from Planck satellite.
