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A Luminous X-Ray Active Galactic Nucleus in the Dwarf–Dwarf Galaxy Merger RGG 66

We present the discovery of a luminous X-ray active galactic nucleus (AGN) in the dwarf galaxy merger RGG 66. The black hole is predicted to have a mass of M _BH ∼ 10 ^5.4 M _⊙ and to be radiating close to its Eddington limit ( L _bol / L _Edd ∼ 0.75). The AGN in RGG 66 is notable both for its prese...

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Bibliografiset tiedot
Päätekijät: Seth J. Kimbrell, Amy E. Reines
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2024-01-01
Sarja:The Astrophysical Journal
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Linkit:https://doi.org/10.3847/1538-4357/ad712d
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