Molecular ions in dense interstellar clouds

Details Molecular ions in dense interstellar clouds Molecular ions in dense interstellar clouds

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..458o&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, May-June 1986, p. 458-464) Soviet Astronomy (ISSN 0038-5301), vol. 30, May-June 1986, p. 274

Astronomy and Astrophysics

Astronomy

1

Abundance, Density Distribution, Interstellar Chemistry, Interstellar Gas, Molecular Clouds, Molecular Ions, Charge Transfer, Cosmic Dust, Cosmic Rays, Ion Production Rates

Scientific paper

Ion kinetics in dense molecular clouds are considered. The molecular ion abundances are calculated using observational data on neutral molecules. H3+, CH3+, HCO+, C2H2+, H3O+, HS+, N2H+ are shown to be the most abundant. As far as ion-dust interactions are concerned, the only essential process is sticking of ions on the grain surface.

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