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Theoretical Studies of Interstellar Isomers
Published online by Cambridge University Press: 04 August 2017
Abstract
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Both observational and theoretical studies of molecular cloud chemistry are hindered by many difficulties which are partially circumvented by studying the relative abundances of isomers synthesized from a common set of chemical precursors. Theoretical studies aimed at understanding interstellar abundance ratios for the isomers HCN/HNC, HCO+/HOC+, CH3CN/CH3NC, and C3H2 have been performed.
- Type
- Interstellar Medium
- Information
- Copyright
- Copyright © Reidel 1987
References
DeFrees, D. J. and McLean, A. D.
1985a, ‘Does carbon-protonated hydrogen cyanide, H2CN+, exist?’, J. Amer. Chem. Soc., 107, 4350.Google Scholar
DeFrees, D. J. and McLean, A. D.
1985b, ‘Ab initio molecular orbital studies of low-energy, metastable isomers of the ubiquitous cyclopropenylidene’, Ap. J. (Letters), submitted.CrossRefGoogle Scholar
DeFrees, D. J., Binkley, J. S., Frisch, M. F., and McLean, A. D.
1985, ‘The lowest singlet and triplet potential energy surfaces of the astrophysically important ion CH2N+
, J. Chem. Phys, manuscript in preparation.Google Scholar
DeFrees, D. J., McLean, A. D., and Herbst, E.
1985, ‘Theoretical investigation of the interstellar CH3NC/CH3CN ratio’, Ap. J., 293, 236.Google Scholar
Jarrold, M. F., Bowers, M. J., DeFrees, D. J., McLean, A. D., and Herbst, E.
1985, ‘A reanalysis of the HCO+/HOC+ abundance ratio in dense interstellar clouds’, Ap. J., in press.Google Scholar
Thaddeus, P., Vrtilek, J. M., and Gottlieb, C. A.
1985, ‘Laboratory and astronomical identification of cyclopropenylidene, C3H2‘, Ap. J. (Letters), in press.Google Scholar
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