Computer Science
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984stin...8427658.&link_type=abstract
Unknown
Computer Science
Abundance, Chondrites, Cosmic Rays, Heavy Elements, Ionization Potentials, Nuclear Fusion, Ariel Satellites, Fractionation, Heao 3, Heavy Nuclei, Interstellar Space, Meteorites, Meteoritic Composition, Solar System
Scientific paper
The elemental composition of the cosmic-ray source is different from that which has been generally taken as the composition of the solar system. No general enrichment of products of either r-process or s-process nucleosynthesis accounts for the differences over the entire range of ultraheavy (Z 30) elements; specific determination of nucleosynthetic contributions to the differences depends upon an understanding of the nature of any acceleration fractionation. Comparison between the cosmic-ray source abundances and the abundances of C1 and C2 chondritic meteorites suggests that differences between the cosmic-ray source and the standard (C1) solar system may not be due to acceleration fractionation of the cosmic rays, but rather to a fractionation of the C1 abundances with respect to the interstellar abundances.
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