Supermassive Star Formation in Magnetized Atomic-cooling Gas Clouds: Enhanced Accretion, Intermittent Fragmentation, and Continuous Mergers

@article{Hirano2021SupermassiveSF,
  title={Supermassive Star Formation in Magnetized Atomic-cooling Gas Clouds: Enhanced Accretion, Intermittent Fragmentation, and Continuous Mergers},
  author={Shingo Hirano and Masahiro N. Machida and Shantanu Basu},
  journal={The Astrophysical Journal},
  year={2021},
  volume={917}
}
The origin of supermassive black holes (with ≳109 M ⊙) in the early universe (redshift z ∼ 7) remains poorly understood. Gravitational collapse of a massive primordial gas cloud is a promising initial process, but theoretical studies have difficulty growing the black hole fast enough. We focus on the magnetic effects on star formation that occurs in an atomic-cooling gas cloud. Using a set of three-dimensional magnetohydrodynamic simulations, we investigate the star formation process in the… Expand

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