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

被引:30
|
作者
Montaigne, H
Geppert, WD [1 ]
Semaniak, J
Österdahl, F
Hellberg, F
Thomas, RD
Af Ugglas, M
Roberts, H
Millar, TJ
Zhaunerchyk, V
Kaminska, M
Al-Khalili, A
Källberg, A
Larsson, M
机构
[1] Stockholm Univ, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden
[2] Royal Inst Technol, Dept Chem, SE-10044 Stockholm, Sweden
[3] Jan Kochanowski Univ Humanities & Sci, Inst Phys, PL-25406 Kielce, Poland
[4] Royal Inst Technol, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden
[5] Univ Manchester, Astrophys Grp, Sch Phys & Astron, Manchester M60 1QD, Lancs, England
[6] Manne Siegbahn Lab, SE-10405 Stockholm, Sweden
来源
ASTROPHYSICAL JOURNAL | 2005年 / 631卷 / 01期
关键词
astrochemistry; ISM : clouds; ISM : molecules;
D O I
10.1086/432253
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 sigma = 1.41 x 10(-15)E(eV)(-1.11) and 4.47 x 10(-16)E(eV) (-1.14) cm(2) for HCS+ and OCS+, respectively. The derived energy dependences of the thermal reaction rate coefficients can be fitted by k(T) 9.7 x 10(-7)(T/300)(-0.57) and 3.5 x 10(-7)(T/300)(-0.62) cm(3) 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.
引用
收藏
页码:653 / 659
页数:7
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