Free Access

Fig. 9.


Gravity (log g) against effective temperature (Teff) for stars observed spectroscopically with AAOmega. Filled circles are radial velocity members while the unfilled ones are non-members. Some radial velocity members are found among the background giant population. In the lower left we show the typical errors.

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.