Free Access
Fig. 3
Brγ emission over the star cluster mass, for the SSCs in the SINFONI fields. As for H2 (see Fig. 2), the Brγ-to-stellar mass ratio is extinction independent. The ratio is normalized to the value for B1.
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.