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

Open Access

Fig. 15.

Cumulative ejected masses of [Na/Fe] and [O/Fe] for 80–500 M_⊙ models calculated at 1/30th Z_⊙. Observations of stars in NGC 5904 are shown as in Fig. 11, adopted from Carretta et al. (2009). The insert includes the wide range of O-enrichment ejected by the 400–500 M_⊙ models during the post-MS.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.