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Fig. 1

image

Upper panels: inner O, C and He abundance distribution in terms of the outer mass fraction for the two stellar models considered in our analysis at Teff ~ 12 000 K. 0TP refers to the expected chemical profiles resulting from a progenitor before the occurrence of the first TP (red dashed line). 3TP corresponds to the case of the chemical profiles resulting from a progenitor at end of the third TP (black solid line).

This figure is made of several images, please see below:

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