Neutral-neutral reactions at the temperatures of interstellar clouds: Ratecoefficients for reactions of atomic carbon, C(P-3), with O-2, C2H2, C2H4 and C3H6 down to 15 K
D. Chastaing et al., Neutral-neutral reactions at the temperatures of interstellar clouds: Ratecoefficients for reactions of atomic carbon, C(P-3), with O-2, C2H2, C2H4 and C3H6 down to 15 K, PCCP PHYS C, 1(9), 1999, pp. 2247-2256
A CRESU (Cinetique de Reaction en Ecoulement Supersonique Uniforme) apparat
us has been used to measure rate coefficients for the reactions of ground-s
tate carbon atoms, C(P-3), with C2H2, C2H4, C3H6 and O-2 at temperatures fr
om 295 down to 15 K. C(P-3) atoms were generated by photolysis of C3O2 at 1
93 nm using an ArF excimer laser and reaction rates were determined by obse
rving the chemiluminescence from NO(B (II)-I-2) which is generated in the r
eaction between C(P-3) atoms and NO2. The rate coefficients for all four re
actions increase as the temperature is lowered, and those for reactions wit
h the unsaturated hydrocarbons exceed 2 x 10(-10) cm(3) molecule(-1) s(-1)
at all temperatures below 300 K. The results confirm that C(P-3) atoms, lik
e C2H radicals and CN radicals, react rapidly with unsaturated hydrocarbons
at very low temperatures. It therefore seems likely that these reactions-a
nd similar ones involving C(P-3) atoms and other hydrocarbons-play an impor
tant role in forming species with long carbon chains in dense interstellar
clouds.