Exploring the formation environment and dynamics of multiple stellar populations in globular clusters through binary systems

Open Access

Fig. 1

m_F814W vs. m_F606W − m_F814W (left) and m_F160W vs. m_F110W − m_F160W CMD (right) of NGC 288 stars. The error bars to the left of each CMD indicate the typical uncertainties for stars with different magnitudes.

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.