Statistics – Computation
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.145..303a&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 145, no. 2, June 1988, p. 303-318. Research supported by the University of
Statistics
Computation
Chemical Fractionation, Lyman Alpha Radiation, Molecular Excitation, Oxygen Isotopes, Photochemical Reactions, Carbon Monoxide, Computational Chemistry, Cosmic Dust, Dissociation, Meteorites, Solar System
Scientific paper
Inferences about the formation of primordial matter in our solar system rest on analysis of the earliest preserved materials in meteorites, of the structure of the solar system today, and of matter in evolving stellar systems elsewhere. The isotope distribution in meteorites suggests that molecular excitation processes similar to those observed today in circumstellar regions and dark interstellar clouds were operating in the early solar nebula. Laboratory model experiments together with these observations give evidence on the thermal state of the source medium from which refractory meteoritic dust formed.
Arrhenius Gustaf
Corrigan M. J.
Fitzgerald Ray W.
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