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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Dettagli Bibliografici

Autori principali:	Benny Trakhtenbrot, Claudio Ricci, Ezequiel Treister, Michael J. Koss, Richard Mushotzky, Kyuseok Oh, Alessandro Peca, Franz E. Bauer, Kriti Kamal Gupta, Tomer Reiss
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2025-01-01
Serie:	The Astrophysical Journal Letters
Soggetti:	Active galactic nuclei High-redshift galaxies Supermassive black holes AGN host galaxies
Accesso online:	https://doi.org/10.3847/2041-8213/ae0d8c
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