Cosmic-ray abundances of elements with atomic number 26 less than or equal to 40 measured on HEAO 3

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Abundance, Cosmic Rays, Heao 3, Nuclear Fusion, Solar System, Ionization, Isotopes, Radiation Sources

Scientific paper

Individual elements in the cosmic radiation of even atomic number (Z) in the interval 26-40 have been resolved and their relative abundances measured. The results are inconsistent with a cosmic-ray source whose composition in this charge interval is dominated by r-process nucleosynthesis. The ratios of cosmic-ray source abundances to solar system abundances in this interval follow the same general correlation with first ionization potential as for the lighter elements, although there are deviations in detail.

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