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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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La firma de las primeras estrellas en hidrógeno atómico en el corrimiento al rojo 20

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
Resumen

La formación de estrellas en el Universo temprano fue suprimida por las diferentes velocidades de la materia. Las simulaciones revelan una señal de hidrógeno mejorada de 21 cm de las primeras estrellas, detectable con radiotelescopios.

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