Physics
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....9..115s&link_type=abstract
IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 9 (A85-22801 0
Physics
Abundance, Cerium, Cosmic Rays, Heavy Nuclei, Radiation Measurement, Tin Isotopes, Barium, Charge Distribution, Heao 3, Nuclear Fusion, Tellurium, Xenon
Scientific paper
Elements with even atomic number (Z) in the interval Z = 50-58 have been resolved in the cosmic radiation using the Heavy Nuclei Experiment on the HEAO-3 satellite. The observation that Sn-50 and Ba-56 are more abundant than Te-52 and Xe-54 indicates a substantial s-process contribution to the cosmic ray source. A significant abundance of Ce-58 provides further support for this finding.
Binns Robert W.
Brewster N. R.
Fickle R. K.
Garrard Thomas L.
Israel Martin H.
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