On the synthesis of c-C3H2 in interstellar clouds

Details On the synthesis of c-C3H2 in interstellar clouds On the synthesis of c-C3H2 in interstellar clouds

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...317l..25a&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 317, June 1, 1987, p. L25-L27.

Astronomy and Astrophysics

Astrophysics

34

Abundance, Hydrocarbons, Interstellar Chemistry, Interstellar Gas, Molecular Clouds, Molecular Ions, Recombination Reactions, Synthesis (Chemistry)

Scientific paper

Following some recent laboratory studies it is proposed that the reaction of C3H+ with H2 is the major source of the cyclic and linear isomers of C3H3+ (i.e., c-C3H3+ and l-C3H3+) in interstellar clouds and that dissociation recombination reactions of these isomeric ions with electrons generate the c-C3H2 molecules (and possibly l-C3H2) recently detected in interstellar clouds.

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