Wind velocities, mass loss rates, radiative acceleration and density for a grid of dynamical models with stellar parameters M_∗ = 1   M_⊙, L_∗ = 5000   L_⊙ and T_eff = 2800   K, a piston velocity of 4 km s^-1 and f_abs = 1.0. The grid covers a range of chemical and optical dust properties, represented by the variables T_c and p, and includes in total 165 dynamical models. The sawtooth-like shape of the boundary between models with and without a wind is a consequence of the discrete number of models in the grid. The radiative acceleration and density is measured at the distance from the star when f_c = 0.5 (where T_d = T_c), averaged over pulsation cycle, and the velocity and mass loss rate are measured at the outer boundary of the model. The over-plotted contours are curves of constant condensation distance (R_c = 2,4,10) using Eq. (10).