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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Bibliographic Details
Main Authors: Ke-Jung Chen, Meng-Yuan Ho, Pei-Cheng Tung
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Online Access:https://doi.org/10.3847/2041-8213/adf18d
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