Other
Scientific paper
Dec 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197..835d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 197, Dec. 1981, p. 835-844.
Other
6
Crystal Surfaces, Diatomic Molecules, Interstellar Chemistry, Interstellar Matter, Oxides, Reactivity, Surface Reactions, Crystal Growth, Nuclear Binding Energy, Particle Interactions, Tables (Data)
Scientific paper
Detailed calculations are made to test the predictions of Duley et al. (1978) concerning the chemical reactivity of interstellar oxide grains. A method is established for calculating interaction energies between atoms and the perfect crystal with or without surface vacancy sites. The possibility of reactions between incident atoms and absorbed atoms is investigated. It is concluded that H2 formation can occur on the perfect crystal surfaces, and that for other diatomic molecules the important formation sites are the Fs and V22-centers. The outline by Duley et al. (1979) of interstellar oxide grain growth and destruction is justified by these calculations.
Denison P.
Williams David. A.
No associations
LandOfFree
Surface chemistry on interstellar oxide grains does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Surface chemistry on interstellar oxide grains, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Surface chemistry on interstellar oxide grains will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1264663