Grain-surface formation of multi-deuterated molecules

Details Grain-surface formation of multi-deuterated molecules Grain-surface formation of multi-deuterated molecules

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.240p..25b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 240, Sept. 15, 1989, p. 25P-29P.

Astronomy and Astrophysics

Astronomy

34

Deuterium Compounds, Interstellar Chemistry, Interstellar Matter, Molecular Clouds, Fractionation, Interstellar Gas, Reaction Kinetics

Scientific paper

A model of the gas-grain interaction describing deuterium chemistry in dense interstellar clouds was extended to include the grain-surface formation of molecules bearing two or more deuterium atoms. It is found that a large degree of fractionation occurs in multideuterated species, which implies that NHD2, for example, should be detectable in hot core regions.

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