Supersonic turbulence, with Mach numbers 1.8 to 4.2 scaling with halo mass, is common in 15 simulated minihalos and fragments their central gas into Jeans-unstable clumps.
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Turbulence in Primordial Dark Matter Halos and Its Impact on the First Star Formation
Supersonic turbulence, with Mach numbers 1.8 to 4.2 scaling with halo mass, is common in 15 simulated minihalos and fragments their central gas into Jeans-unstable clumps.