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Dissociative Recombination of the Thioformyl (HCS+) and Carbonyl Sulfide (OCS+) Cations

Authors :
Tom J. Millar
H. Roberts
Vitali Zhaunerchyk
Wolf D. Geppert
J. Semaniak
A. Al-Khalili
Mats Larsson
F. Österdahl
Fredrik Hellberg
H. Montaigne
Richard D. Thomas
Magdalena Kaminska
Anders Källberg
M. af Ugglas
Source :
The Astrophysical Journal. 631:653-659
Publication Year :
2005
Publisher :
American Astronomical Society, 2005.

Abstract

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 C–S 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 = 1.41 × 10-15E(eV)-1.11 and 4.47 × 10-16E(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) = 9.7 × 10-7(T/300)-0.57 and 3.5 × 10-7(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.

Details

ISSN :
15384357 and 0004637X
Volume :
631
Database :
OpenAIRE
Journal :
The Astrophysical Journal
Accession number :
edsair.doi...........25744a90ce6e799b7f2554773c8079ef
Full Text :
https://doi.org/10.1086/432253