Fig. 1.
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Volume density profiles of individual stellar (NSC) and BH (BW) components (top panel) and cumulative mass profiles of the same (bottom panel) for NGC205 NSC + BW model. The full lines represent initial profiles for the BH and stellar components, and dashed lines represent the same (in corresponding colors) at designated times in Myr. The vertical brown line represents the sphere of influence (rinfl1) of the IMBH for initial distribution, and the vertical gray line showcases the effective radius of the NSC.
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