  This study concerns the consistency of the tachyon warm inflationary models.
A linear stability analysis is performed to find the slow-roll conditions,
characterized by the potential slow-roll (PSR) parameters, for the existence of
a tachyon warm inflationary attractor in the system. The PSR parameters in the
tachyon warm inflationary models are redefined. Two cases, an exponential
potential and an inverse power-law potential, are studied, when the dissipative
coefficient $\Gamma=\Gamma_0$ and $\Gamma=\Gamma(\phi)$, respectively. A
crucial condition is obtained for a tachyon warm inflationary model
characterized by the Hubble slow-roll (HSR) parameter $\epsilon_{_H}$, and the
condition is extendable to some other inflationary models as well. A proper
number of e-folds is obtained in both cases of the tachyon warm inflation, in
contrast to existing works. It is also found that a constant dissipative
coefficient $(\Gamma=\Gamma_0)$ is usually not a suitable assumption for a warm
inflationary model.
