Insights for Early Massive Black Hole Growth from JWST Detection of the [Ne v] λ3427 Emission Line
We use the narrow [Ne v] λ 3427 emission line detected in the recently published JWST spectra of two galaxies, at z ≃ 6.9 and 5.6, to study the key properties of the active galactic nuclei (AGN) and the supermassive black holes (SMBHs) in their centers. Using a new empirical scaling linking the $\l...
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| Principais autores: | , , , , , , , , , |
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| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
IOP Publishing
2025-01-01
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| Serier: | The Astrophysical Journal Letters |
| Fag: | |
| Online adgang: | https://doi.org/10.3847/2041-8213/ae0d8c |
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