First models of the s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver

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Fig. 11.

Observed abundances from Madonna (2018) of PN NGC 3918 (open triangles) and NGC 7027 (filled squares) alongside the best fitting of our overabundance results (lines and filled dots). In grey are shown the uncertainties for each of the measurements.

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