Dynamical status of Globular cluster NGC 362

The study of the dynamical status of the globular cluster NGC362 is presented using the spatial distribution of Blue Straggler Stars (BSSs). A significant cluster area is covered using multi-wavelength high-resolution space and ground-based data. The cluster members are selected using HST and Gaia EDR3 proper motion data sets. Using members of the cluster, the cluster’s projected density profile is created. The cluster’s radius is determined using the projected density profile. The BSS radial distribution has been used to determine the cluster’s dynamic age.