Fig. 5
Stellar distributions of runs with a full eos with nad = 1010 cm−3 (C10f, C10fd) and 109 cm−3 (C1f). The transitions to γ = 5∕3, 7∕5, and 1.1occur at nad, 30 nad, and 30 000 nad. Using a higher sink density threshold (C10fd) results in fewer low-mass stars but does not change the peak of the stellar distribution. Decreasing nad by a factor ten increases the peak mass by ~10.
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