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Directly Tracking the Rebrightening of a Supermassive Black Hole Accretion Disk

Accretion onto supermassive black holes (SMBHs) powers the most luminous persistent sources in the Universe, the so-called active galactic nuclei, whose emission is characterized by two distinct spectral components: thermal optical/ultraviolet (UV) radiation from an optically thick accretion disk an...

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Furkejuvvon:
Váldodahkkit: Riccardo Middei, Emanuele Nardini, Chris Done, Elisabeta Lusso, F. Vagnetti, G. Risaliti, E. Piconcelli, S. Bianchi, G. Matzeu, A. Trindade Falcão, D. Ł. Król, M. Perri, A. Maselli, K. Horne, J. V. Hernández Santisteban
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: IOP Publishing 2026-01-01
Ráidu:The Astrophysical Journal
Fáttát:
Active galactic nuclei
Active galaxies
Liŋkkat:https://doi.org/10.3847/1538-4357/ae6f0e
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