Fig. 1
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Initial half-mass density ρh, computed at the initial half-mass radius rh, is expressed as a function of the initial number of stars N. The figure has been reproduced from Arca Sedda et al. (2023, 2024b,a) and adapted to include a color bar with the logarithm of the average half-mass radius. We include other simulations and the new ones presented in this paper.
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