Explosive nucleosynthesis and meteoritic isotope anomalies

Details Explosive nucleosynthesis and meteoritic isotope anomalies Explosive nucleosynthesis and meteoritic isotope anomalies

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....74..247c&link_type=abstract

Astronomy and Astrophysics, vol. 74, no. 2, Apr. 1979, p. 247-249.

Astronomy and Astrophysics

Astrophysics

5

Aluminum 26, Carbonaceous Chondrites, Interstellar Chemistry, Nuclear Fusion, Oxygen 17, Abundance, Carbon, Combustion, Fluorine Isotopes, Helium, Iron Isotopes, Neon, Neutrons, Sodium 22, Stellar Evolution

Scientific paper

A reconsideration of neutron absorption by Fe-56 in explosive C burning, in the light of the study by Howard et al. (1972), leads to the conclusion that more O-17 and less Al-26 are likely to be produced than hitherto thought. The anomalous O-16 and Al-26 detected in carbonaceous chondrites are therefore more likely to have been produced in explosive He burning.

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