Fig. 3.
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Same as Fig. 2, but with a logarithmic scale on both axes, and starting only from R = 1″. The regression line shown in magenta is computed from the red dots displayed here, discarding the dot at R ≃ 4 kpc. The black line shows the power law with an index −1.8, corresponding to the average SB profiles of the blobs studied by Borisova et al. (2016). The stellar profile is shown in cyan.
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