Are Single-zone Emission Models Sufficient to Explain GRB 220426A and GRB 230812B?
Gamma-ray bursts (GRBs) are the Universe’s most energetic phenomena (isotropic luminosity ∼10 ^51 –10 ^54 erg s ^−1 ) lasting for a very short duration (∼milliseconds—a few seconds). Even after an average of one GRB detected per day, their emission mechanism remains contentious. Inferences drawn fro...
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| Principais autores: | , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
IOP Publishing
2026-01-01
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| coleção: | The Astrophysical Journal |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.3847/1538-4357/ae6809 |
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