Fig. A.6
Theoretical interpretation of the post-AGB stars GLMP 334 ([Fe/H] = − 0.4; Teff = 7400 K; log g = 1.4) with = 5 M⊙ models. Three 13C-pocket efficiencies are shown: cases ST-IMS × 4 (solid line), ST-IMS × 2 (dotted thin line) and ST-IMS (dotted thick line). Note that a different 13C-pocket notation is adopted for IMS stars, because they have a smaller He-intershell than low-mass AGBs, with a smaller 13C-pocket (see Bisterzo et al. 2010). None of these solutions agrees with the observations.
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