Fig. 16
Stellar density profiles of the C-type (triangles) and M-type (squares) AGB and RGB (stars) sources in each region in the multi-resolution grid (Fig. 15). The stellar density has been normalised to account for the varying area of each grid region. The horizontal lines at 1.66 and 0.48 represent the level of the remaining foreground contamination in the M- and C-type samples respectively. The vertical line at 4 kpc marks the limit of the detectable stellar component of NGC 6822.
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