We have investigated the chemistry of C + H + 3 forming CH + , CH + 2 , and CH + 3 . These reactions are believed to be some of the key gas-phase astrochemical processes initiating the formation of organic molecules in molecular clouds. For this work we have constructed a novel merged fast-beams apparatus which overlaps a beam of molecular ions onto a beam of ground-term neutral atoms. Here we describe the apparatus in detail and present cross section data for forming CH + and CH + 2 at relative energies from ≈ 9 meV to ≈ 20 and 3 eV, respectively. Measurements were performed for statistically populated C( 3 P J ) in the ground term reacting with hot H + 3 (at an internal temperature of ∼ 2, 550 K). Using these data we have derived rate coefficients for translational temperatures from ≈ 72 K to ≈ 2.3 ×10 5 and 3.4 ×10 4 K, respectively. For the formation of CH + 3 we are able only to put an upper limit on the rate coefficient. Our results for CH +