Abstract
Photoionization yield curves have been obtained for the major ions from CH3SH. Auxiliary studies with selectively deuterated species reveal that CD3S+ has a slightly lower threshold than CD2SH+ from CD3SH; but CH2SD+ has a lower threshold than CH3S+ from CH3SD. An analysis of alternative interpretations is presented. The isotopic studies also imply that CH2S+ is more stable than HCSH+, and HCS+ is more stable than CSH+. The value ΔH°f,0(HCS+)≤259.2±0.9 kcal/mol obtained in this study is in good agreement with a bracketed proton affinity for CS, but differs significantly from a recent ab initio calculation. This result confirms the view that HCS+ can be formed in interstellar clouds by exothermic reactions. The reaction CH3S+/CH2SH+→HCS++H2 proceeds weakly at threshold, and much more strongly after overcoming an activation barrier of ∼0.9 eV.
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Dates
Type | When |
---|---|
Created | 22 years, 6 months ago (Feb. 28, 2003, 11:32 a.m.) |
Deposited | 1 year, 6 months ago (Feb. 9, 2024, 7:36 p.m.) |
Indexed | 1 year, 6 months ago (Feb. 11, 2024, 4:43 a.m.) |
Issued | 42 years, 8 months ago (Dec. 1, 1982) |
Published | 42 years, 8 months ago (Dec. 1, 1982) |
Published Print | 42 years, 8 months ago (Dec. 1, 1982) |
@article{Kutina_1982, title={Photoionization mass spectrometry of CH3SH, CD3SH, and CH3SD: Heats of formation of CH3S+(CH2SH+), CH2S+, CH2S, and HCS+}, volume={77}, ISSN={1089-7690}, url={http://dx.doi.org/10.1063/1.443756}, DOI={10.1063/1.443756}, number={11}, journal={The Journal of Chemical Physics}, publisher={AIP Publishing}, author={Kutina, R. E. and Edwards, A. K. and Goodman, G. L. and Berkowitz, J.}, year={1982}, month=dec, pages={5508–5526} }