Fig. 14
Download original image
Production of Sr, Y, Ba and La is shown for nucleosynthesis models of fast-rotating massive stars for different amounts of22Ne consumed by the 22Ne(α,n)25Mg reaction rate (top). The trends of [Sr/Y] (middle) and [Ba/La] (bottom) are shown with the stars observed in this work with current error ranges if available, in comparison with the r-process star CS22892-052 (Sneden et al. 2003, 2009).
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.