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Fig. 3.
Equilibrium abundances of the 12C and 14N nuclides (dashed and dotted lines) and the cumulative neutrino fluxes of the 13N and 15O disintegrations, ϕ13N and ϕ15O (solid and dot-dashed lines). They are drawn as a function of the temperature, for three SSMs with different chemical mixtures, as given in the legend.
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