Abundance pattern in terms of the ejecta of the 6 M_⊙ models computed with the Blo95 wind prescription, and assuming dilution with a low-mass star envelope (see Fig. 11 and main text for details), with η = 0.02, (dotted line), η = 0.04 (dashed line), and η = 1 (solid line). Abundances from the Z = 2 × 10⁻⁵, 6 M_⊙ model by Iwamoto (2009) are shown by the grey solid line. Symbols represent the observed abundances of CS29528-041.