'Primary' elements in H-burning

Details 'Primary' elements in H-burning 'Primary' elements in H-burning

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..53..217c&link_type=abstract

Astrophysics and Space Science, vol. 53, no. 1, Jan. 1978, p. 217-221.

Astronomy and Astrophysics

Astrophysics

2

Abundance, Hydrogen, Nuclear Fusion, Stellar Evolution, Beryllium 7, Carbon 13, Convective Flow, Equilibrium Equations, Nitrogen 15, Oxygen 17, Turbulent Mixing

Scientific paper

The behavior of intermediate nuclei taking part in H-burning is analyzed. Comparing time scales for equilibrium with the time scale of convective mixing, it is found that Be-7, C-13, N-15, and O-17 cannot be assumed everywhere as bona fide secondary elements in stellar evolutionary computations. Some consequences of the onset of CNO burning are also discussed.

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