Electronic Resource
Springer
Astrophysics and space science
53 (1978), S. 217-221
ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract The behaviour of intermediate nuclei taking part in H-burning is analysed. Comparing time scales for equilibrium with the time scale of convective mixing, we find that Be7, C13, N15, O17 cannot be assumed everywhere asbona fide secondary elements in stellar evolutionary computations. Some consequences of the onset of CNO burning are also discussed.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00645915
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