Determining the dynamical age of the LMC globular cluster NGC 1835 using the ‘dynamical clock’ - Star density profile and blue straggler stars

Open Access

Fig. 6.

Normalised cumulative radial distributions of BSSs (solid blue line) and RGB stars (dashed red line) in one of the random realisations used to estimate the $A_{rh}^{+}$ $A^+_{\mathrm{rh}}$ parameter in NGC 1835. The area enclosed between the two curves corresponds to the value of $A_{rh}^{+}$ $A^+_{\mathrm{rh}}$ (see the label).

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.