Fig. 6
Li abundance vs. stellar effective temperature for the sample stars. The four best-fit candidates are indicated by their HD numbers. The average Li abundances for 0.1 Gyr and 2.0 Gyr open clusters (Pleiades and Blanco1, and Hyades, Praesepe, Coma Ber, and NGC 6633) in three ranges of Teff are also shown. The data are taken from Sestito & Randich (2005).
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.