All Tables

Table 1: Pre-shock, shock front, and excursion ( $\equiv$ post-shock) gas temperature and number density as a function of position in the envelope and shock strengths. M is the Mach number (= $v_{\rm sh}$ / $v_{\rm esc}$ ) associated with each shock speed.
Table 2: Chemical species considered in the present inner wind model: elements are He, H, O, C, N, Si, and S.
Table 3: Species abundances in the post-shock gas at 1 $R_{\star }$ for TE calculations and non-equilibrium chemistry.
Table 4: Abundances between 1 $R_{\star }$ to 5 $R_{\star }$ for molecules common to all AGB, whatever the C/O ratio.
Table 5: Species present in the inner wind of S stars as a function of C/O ratios and position.