Fig. 3
Comparison of the abundance of [(C+N)/Fe]. (i) For the sample of EMP stars studied in the framework of the Large Program First Stars: filled blue squares for unmixed RGB stars, filled red diamonds for mixed RGB’s, and filled black circles for the turnoff stars (no EMP turnoff stars appear in this figure, because it was not possible to measure the nitrogen abundance in these stars Bonifacio et al. 2009); (ii) for CEMP-no (open green crosses); (iii) for CEMP-s (open green circles), and (iv) for the three low-[Sr/Ba] giants here studied (open pink star symbols). These three low-[Sr/Ba] stars are located in the region generally occupied by the carbon-rich stars.
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.