The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity

Tables of ejected masses and net wind yields for stellar evolution models calculated at various metallicities for a range of initial masses associated with the published journal article Higgins et al. (2025). Properties of these models are provided in separate tables, outlining masses and burning timescales at the end of core H-burning and core He-burning phases.

External deposit with Zenodo.