General dissipative coefficient in warm intermediate and logamediate
  inflation
  We study a general form for the dissipative coefficient
$\Gamma(T,\phi)=C_\phi\,T^{m}/\phi^{m-1}$ in the context of warm intermediate
and logamediate inflationary universe models. We analyze these models in the
weak and strong dissipative regimes. In the slow-roll approximation, we
describe in great detail the characteristics of these models. In both regimes,
we use recent data from the WMAP nine-year data and Planck data to constrain
the parameters appearing in our models.
