Thermal Evolution of the Intergalactic Medium due to Lyα Photons during the Cosmic Dawn
The first star-forming objects that formed at high redshifts during the cosmic dawn (CD) also emitted photons between Ly α and Lyman-limit frequencies. These photons are instrumental in coupling the spin temperature of the neutral hydrogen (H i ) atoms with the kinetic temperature of the intergalact...
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| Autores principales: | , , |
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| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
IOP Publishing
2024-01-01
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| Colección: | The Astrophysical Journal |
| Materias: | |
| Acceso en línea: | https://doi.org/10.3847/1538-4357/ad84ec |
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