Fig. 3.
Top: radial star count profiles for the MS/HeB (a), AGB (b), and RGB (c) stars in NGC 300. Circles and squares indicate the profiles along the major and minor axes of the galaxy, respectively. The approximate background levels of each population are marked by shaded regions. Bottom: same as top but after background subtraction. Numbers in each panel indicate field IDs. Dashed lines in panel (d) represent the exponential fit of the major and minor axis profiles. (g) Relative densities of MS/HeB and AGB stars with respect to RGB stars along the major axis.
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