We present a combined experimental and theoretical study on the formation processes and ionization energies of small organo-silicon molecules of the formula SiC 2 H x (x = 0, 1, 2). These organic molecules are considered important benchmark systems in understanding the formation of silicon-and carbon-bearing grains in the outflow of carbon stars. The studies identify four distinct (hydrogenated) silicon-carbon molecules together with their ionization energies: c-SiC 2 [9.75 ± 0.10 eV; 9.83 ± 0.05 eV], l-HCCSi [7.00 ± 0.05 eV], c-SiC 2 H [7.27 ± 0.05 eV], and c-SiC 2 H 2 [9.05 ± 0.05 eV; 8.96 ± 0.05 eV] with numbers in italics depicting computed data. Implications of these results to the non-equilibrium chemistry in shocked regions of circumstellar envelopes of carbon stars are also discussed.