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2005ApJ...631..653M - Astrophys. J., 631, 653-659 (2005/September-3)

Dissociative recombination of the thioformyl (HCS+) and carbonyl sulfide (OCS+) cations.

MONTAIGNE H., GEPPERT W.D., SEMANIAK J., OSTERDAHL F., HELLBERG F., THOMAS R.D., AF UGGLAS M., ROBERTS H., MILLAR T.J., ZHAUNERCHYK V., KAMINSKA M., AL-KHALILI A., KALLBERG A. and LARSSON M.

Abstract (from CDS):

Branching ratios and absolute cross sections have been measured for the dissociative recombination of HCS+ and OCS+ at the CRYRING ion storage ring. In the case of OCS+, the channel leading to CO+S (83%) dominates, whereas the other exoergic pathways leading to CS+O (14%) and C+SO (3%) are of lesser importance. In the case of HCS+, fracture of the CS bond is predominant (81%), with the production of H+CS accounting for the remainder (19%). The cross section of the reaction could be fitted by the expressions σ=1.41x10–15E(eV)–1.11 and 4.47x10–16E(eV)–1.14 cm2 for HCS+ and OCS+, respectively. The derived energy dependences of the thermal reaction rate coefficients can be fitted by k(T)=9.7x10–7(T/300)–0.57 and 3.5x10–7(T/300)–0.62 cm3 s–1 for HCS+ and OCS+, respectively. We use these data to perform model calculations on the HCS+/CS abundance ratio in dark clouds and find that the models using the UMIST and Ohio State University databases have even more difficulty in accounting for the large observed ratio.

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Journal keyword(s): Astrochemistry - ISM: Clouds - ISM: Molecules

Simbad objects: 3

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