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Updated: May 5, 2026

Measurement and Analysis of Atomic Hydrogen and Diatomic Molecular AlO, C2, CN, and TiO Spectra Following Laser-induced Optical Breakdown
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赤い偏移20で原子水素で最初の星のサイン

Eli Visbal1, Rennan Barkana, Anastasia Fialkov

  • 1Jefferson Laboratory of Physics, Harvard University, Cambridge, Massachusetts 02138, USA. evisbal@fas.harvard.edu

Nature
|June 23, 2012
PubMed
まとめ

初期の宇宙の星形成は,異なる物質速度によって抑制された. シミュレーションでは,最初の星から21cmの強化された水素信号が発せられ,これはラジオ望遠鏡で検出できる.

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