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Fig. 2
Density profiles of the star cluster (black dashed line), of the residual (solid lines), and initial (dash-dotted lines) gas for different SFEgl in scaled physical units. A total stellar mass M⋆ = 3000 M⊙ and a 3D half-mass radius rh = 1 pc are assumed. Note that the stellar density profile is a Plummer profile.
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