Fig. 5
Radial variation of the stellar surface density for the MB samples in blue. Vertical red lines show the 1.2 and 3 kpc completeness limits. Green dots show the points used for the exponential fit, avoiding those around the overdensity location. The exponential fit is plotted in magenta, with the hR and Σ⊙ parameters expressed in pc and ⋆/pc2, respectively.
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