Dissociative recombination of interstellar ions: electronic structure calculations for HCO(+)

Details Dissociative recombination of interstellar ions: electronic structure calculations for HCO(+) Dissociative recombination of interstellar ions: electronic structure calculations for HCO(+)

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985masa.conf..575k&link_type=abstract

In: Molecular astrophysics: State of the art and future directions; Proceedings of the Advanced Research Workshop, Bad Windsheim

Astronomy and Astrophysics

Astrophysics

1

Cosmochemistry, Formyl Ions, Interstellar Space, Recombination Reactions, Self Consistent Fields, Dissociation, Molecular Ions, Molecular Structure

Scientific paper

A study of the interstellar formyl ion HCO(+) is the first attempt to investigate dissociative recombination for a triatomic molecular ion using an entirely theoretical approach. A number of fairly extensive electronic structure calculations that were performed to determine the reaction mechanism of the e-HCO(+) process are described. Similar calculations for the isoelectronic ions HOC(+) and HN2(+) are in progress.

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