Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC

Open Access

Fig. 8.

Total amount of mass ejected for 4 species. Fe refers to the isotopes ⁵²Fe through ⁵¹Fe and the ⁵⁶Ni that decays into ⁵⁶Fe. It is worth noting the peculiar behavior of ¹⁴N for Z = 0.001, resulting from the specific interplay between the dredge-up history and the final fate of these tracks (see text for more details).

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