Photodissociation of CH 3 NH 2 + has been studied using the DC sliced ion imaging technique and ab initio calculations in order to understand the formation of HCNH + , an important molecule in Titan's ionosphere. Our experimental and theoretical observations show that hydrogen loss from CH 3 NH 2 + has two channels: one giving rise to the triplet species CH 3 NH + , while the other product is CH 2 NH 2 +. The latter then decomposes further to form HCNH +. H 2 loss from CH 3 NH 2 + has only one channel, yielding CH 2 NH +. This species further loses H to form HCNH +. The branching ratio of the H, H 2 , and H+H 2 loss channels is found to be 4.2:1:2.5. This is ascribed to the fact that, at these energies, the H loss has one stable triplet product channel, while most of the H 2 loss product further decomposes to HCNH + .