High temperatures and densities analytical thermodynamic properties are derived for the general Buckingham Exp(α, m) fluids by: a) using the Ross analytical (RA) variation perturbation theory developed by Sun [Mol. Phys. 105 (2007) 3139] for multi-Yukawa potentials; b) using a two-Yukawa potential matching the Exp(α, m), and c) introducing correcting terms which account for the discrepancies between the original Exp(α, m) potential and its two-Yukawa representation. We call this method the Ross analytical corrected theory (RAC), which leads to analytic expressions for the excess Helmholtz free energy, excess internal energy and the compressibility factor Z (i.e. the equation of state). They are valid at high temperatures and densities, since they are obtained from the Ross theory, which extends the range of validity of perturbation theories to higher densities. The matching two-Yukawa potential can also be considered as a reference potential for a first-order perturbation theory, which after further simplification leads to an analytic augmented van der Waals (avdW) theory for the above thermodynamic properties of the Exp(α, m) fluids. For the Exp(11.5, 6) and Exp(14.5, 6) fluids, the excess internal energy, compressibility factor Z and reduced pressure obtained from the RAC and avdW theories are compared with Monte Carlo (MC) simulation results corresponding to both the Exp and TY potentials. The overall accuracy of the RAC and avdW theories for the Exp(11.5, 6) fluid is also assessed in comparison to the Ross numerical (RN) theory (called also MCRSR for Mansoori, Canfield, Rasaiah, Stell and Ross) and to more complex methods such as the KLRR-T (Kang, Lee, Ree, Ree-Theostar) and the HMSA/C (hypernetted mean spherical approximation with Chebyshev approximants) theories, which require more extensive numerical calculations.