X-Ray Weak Active Galactic Nuclei from Super-Eddington Accretion onto Infant Black Holes
A simple model for the X-ray weakness of James Webb Space Telescope–selected broad-line active galactic nuclei (AGNs) is proposed under the assumption that the majority of these sources are fed at super-Eddington accretion rates. In these conditions, the hot inner corona above the geometrically thin...
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| Auteurs principaux: | , |
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| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
IOP Publishing
2024-01-01
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| Collection: | The Astrophysical Journal Letters |
| Sujets: | |
| Accès en ligne: | https://doi.org/10.3847/2041-8213/ad90e1 |
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