Issue |
A&A
Volume 365, Number 2, January 2001
|
|
---|---|---|
Page(s) | 241 - 247 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361:20000026 | |
Published online | 15 January 2001 |
Rate coefficients for the reactions of
C(
P
) atoms with
C2H2,
C2H4,
CH3C
CH and
H2C
C
CH2 at
temperatures down to 15 K
School of Chemistry, The University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
Corresponding author: I. W. M. Smith, i.w.m.smith@bham.ac.uk
Received:
29
August
2000
Accepted:
11
October
2000
Rate coefficients for the reactions of ground state carbon atoms, C(3PJ), with the
four unsaturated hydrocarbons C2H2, C2H4, and
have been measured
at temperatures down to 15 K. The experiments have been performed in a continuous flow
CRESU (Cinétique de Réaction en Écoulement Supersonique Uniforme) apparatus using
pulsed laser photolysis of C3O2 to generate C(3PJ) atoms and laser-induced fluorescence in the
vacuum ultraviolet to observe the kinetic decays of the atoms and hence determine the rate
coefficients. All four reactions are found to occur at rates close to the collision-determined
limit and the rates show at most a very mild dependence on temperature. It is argued that
normally these reactions proceed along a reaction path with no barrier to form a strongly
bound energised adduct, which subsequently eliminates an H atom to form the reaction
products. The rates of the reactions of C(3PJ) atoms with larger unsaturated hydrocarbons are
discussed. Finally, the relevance of the results for the chemistry of dense interstellar clouds is
considered.
Key words: molecular data -molecular processes -methods: laboratory -ISM: clouds
© ESO, 2001
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