The role of H+ and H+3 ions in the degradation of interstellar molecules

David Smith, Patrik Spanel, T. J. Millar

Research output: Contribution to journalArticlepeer-review

21 Citations (Scopus)

Abstract

The results of recent laboratory studies of the reactions of H+ and H+3 with a number of molecular gases are interpreted from the viewpoint of interstellar chemistry. Many of the reactions of these ions result in the ionization and fragmentation of neutral reactant gases. Pseudo-time-dependent calculations of the chemistry in dense molecular clouds indicate that molecular abundances are reduced by the inclusion of such reactions, but generally by less than a factor of 5.

Original languageEnglish
Pages (from-to)31-34
Number of pages4
JournalMonthly Notices of the Royal Astronomical Society
Volume266
Issue number1
DOIs
Publication statusPublished - 01 Jan 1991
Externally publishedYes

Keywords

  • ISM: Abundances
  • ISM: Clouds
  • ISM: Molecules
  • Molecular processes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'The role of H+ and H<sup>+</sup><sub>3</sub> ions in the degradation of interstellar molecules'. Together they form a unique fingerprint.

Cite this