Production and loss of HC3N in interstellar clouds - Some relevant laboratory measurements

Details Production and loss of HC3N in interstellar clouds - Some relevant laboratory measurements Production and loss of HC3N in interstellar clouds - Some relevant laboratory measurements

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.219...89k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 219, March 1, 1986, p. 89-94. Research supported by the

Astronomy and Astrophysics

Astronomy

21

Acetylene, Cyano Compounds, Cyanoacetylene, Interstellar Chemistry, Ionic Reactions, Molecular Collisions, Reaction Kinetics, Recombination Reactions

Scientific paper

The results of recent selected ion flow tube (SIFT) experiments on the ion-molecule chemistry of cyanoacetylene are considered in the context of the chemistry of HC3N in the interstellar environment. Important errors revealed by this SIFT investigation, following an earlier flowing afterglow study in the authors' laboratory, have led to a different perception of the ion-molecule chemistry that HC3N may undergo in interstellar clouds. It is now evident that insertion and association occur in the reactions of hydrocarbon ions with HC3N.

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