Other
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3..163s&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Rar Conf., Vol. 3 p 163-166 (SEE N85-34862 23-93)
Other
Abundance, Cosmic Rays, Galactic Radiation, Supernovae, Helium, Hydrogen, Interstellar Matter, Interstellar Radiation, Mathematical Models, White Dwarf Stars
Scientific paper
A model of cosmic-ray origin is suggested which aims to account for some salient features of the composition. Relative to solar abundances, the Galactic cosmic rays (GCR) are deficient in hydrogen and helim (H and He) by an order of magnitude when the two compositions are normalized at iron. Our conjectural model implicates supernovae of Type I (SN-I) as sources of some of the GCR. SN-I occur approximately as often as SN-II, through their genesis is thought to be different. Recent studies of nucleosynthesis in SN-I based on accreting white dwarfs, find that the elements from Si to Fe are produced copiously. On the other hand, SN-I are virtually devoid of hydrogen, and upper limits deduced for He are low. If SN-I contribute significantly to the pool of GCR by injecting energetic particles into the interstellar medium (ISM), then this could explain why the resulting GCR is relatively deficient in H and He. A test of the model is proposed, and difficulties are discussed.
Shapiro Marjorie
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