Theoretical investigation of the interstellar CH3NC/CH3CN ratio
Calculations have been performed to determine the abundance ratio of the metastable isomer CH3NC to the stable isomer CH3CN in dense interstellar clouds. According to gas phase, ion-molecule treatments, these molecules are both synthesized via protonated ion precursors. A calculation has been made o...
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Veröffentlicht in: | The Astrophysical journal 1985-06, Vol.293 (1), p.236-242 |
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Format: | Artikel |
Sprache: | eng |
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