Fig. 6
Comparison of the predicted Li abundance vs. metallicity relations (lines) for two models (tm03T43 and tm03T45) with the observed data (symbols) of warm metal-poor dwarfs taken from Thorburn (1994; Teff > 6100 K; crosses), Ryan et al. (1999; open squares), Asplund et al. (2006; open circles), and Meléndez et al. (2010; Teff > 6100 K; filled squares). The horizontal dashed line indicates the primordial (CMB+BBN) Li abundance of 2.64.
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.