Astrophysical implications of the isotopic composition of cosmic rays

Details Astrophysical implications of the isotopic composition of cosmic rays Astrophysical implications of the isotopic composition of cosmic rays

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icrc....1..367m&link_type=abstract

In: International Cosmic Ray Conference, 14th, Munich, West Germany, August 15-29, 1975, Conference Papers. Volume 1. (A76-26851

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Abundance, Astrophysics, Chemical Composition, Cosmic Rays, Energy Spectra, Isotopes, Balloon Sounding, Carbon Isotopes, Helium Isotopes, Milky Way Galaxy, Nitrogen Isotopes, Nuclear Fusion, Oxygen Isotopes, Particle Production, Propagation, Spallation

Scientific paper

This paper considers some of the astrophysical consequences of recent cosmic-ray isotope measurements in the charge range between 4 and 26 for energies of 200 to 600 MeV/amu. Using a simple exponential path-length propagation model, the isotopic and chemical compositions are extrapolated observed back to the cosmic-ray source. With the possible exception of neon, all the results are consistent with the current understanding of cosmic-ray propagation and source composition. Some implications of the isotopic data as to the nature of the source are discussed.

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