Chemische Berichte · 1989 · 56 citations · 23 references
Natural SciencesChemistryAnalytical ChemistryComputational ChemistrySpectroscopyInterstellar ChemistryInterstellar GasInterstellar MoleculesMass SpectrometryMolecular Formation PathwaysSulfur ChemistryAb Initio CalculationsAb Initio Molecular CalculationsChemical Composition Of Interstellar GasGas-phase ReactionsInterstellar Gas-phase ChemistryInterstellar Molecule FormationInterstellar RadicalsSpectroscopy Of Interstellar Molecules
Abstract The title compounds are generated and characterized in the gas phase by mass spectrometric methods (neutralization‐reionization mass spectrometry), and for dicarbon sulfide the experimental results are supported by ab initio MO calculations (HF/6‐31G * ).
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