Fig. 2.
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Stellar density profiles with 0, 107, 108, 109, and 1010 years passed for (a) M• = 108 M⊙, (b) M• = 109 M⊙, and (c) M∙ = 1010 M⊙. The purpose of these profiles is to provide an idea of how stellar density profiles can change over time as the depletion of stars from collisions is balanced by the continuous formation of new stars.
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