Fig. 10
Download original image
Age-metallicity relation (AMR) for star clusters in GAMA 526784 (red) compared to the star cluster population in the Large Magellanic Cloud (grey scatter points), along with the bursting model of Pagel & Tautvaisiene (1998) to explain the LMC cluster population. The figure illustrates that GAMA 526784 had an evolution similar to that of the LMC, with a prolonged period of quiescence followed by a recent burst of star cluster formation.
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.