Fig. 2
Comparison of the effects of different observational biases (black) on the unbiased local two-dimensional (2D) density distribution (grey) for star clusters consisting of 1 k (dashed) and 10 k (solid) particles with a King parameter of W0 = 12. a) Resolution limit of the IRAC camera of the Spitzer Space Telescope. b) Cutout of the densest inner 0.5 pc. c) Combined effects a) and b).
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