Differential chemical abundances of Si, Fe, Ni, and Ca of the analyzed stars in the tidal tails of the Hyades and NGC 2632. The color code is the same as in Fig. 7. Red crosses indicate stars identified as kinematic outliers. Shadowed regions represent the cluster signature: 1σ (dark gray) and 3σ (light gray) dispersion. Numbered stars are discussed in the text.
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.