In the interstellar clouds, a number of oxygen-containing organic compounds
such as alcohols and carbonium compounds have been observed. In order to i
nvestigate the role of grain processes for the formation and destruction of
these compounds, thin films of acetone and 2-propanol deposited on the cop
per metal surface at 13 K were reacted with cold gas-phase H atoms (similar
to 27 K). The major products from acetone were found to be methane and alc
ohols (smaller than propanol). 2-propanol was not detected as a reaction pr
oduct. This indicates that the disproportionation reaction is the major pro
cess, but that the recombination one is minor in the reaction of H with the
intermediate (CH3)(2)COH radical. The reaction of H with 2-propanol led to
the formation of methane, alcohols, and acetone as major products. The dep
endences of the film thickness, reaction time, and reaction temperature on
the product yields were measured. It is suggested that the diffusion length
of the H atoms in the 2-propanol film is longer than that in the acetone h
im, and consequently greater product yields were obtained for 2-propanol th
an for acetone with thicker sample films. The temperature-independent produ
ct yields in the range of 13-80 K invoke the tunneling processes in the rea
ctions.