Formation of Supersonic Turbulence in the Primordial Star-forming Cloud
We present new simulations of the formation and evolution of the first star-forming cloud within a massive minihalo of mass of 1.05 × 10 ^7 M _⊙ , carried out using the GIZMO code with detailed modeling of primordial gas cooling and chemistry. Unlike previous studies that simulated the formation of...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/adf18d |
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