The High-redshift Blazar MG3 J163554+3629: Physical Properties and the Enigma of Its Unexpected Supermassive Black Hole Growth

The High-redshift Blazar MG3 J163554+3629: Physical Properties and the Enigma of Its Unexpected Supermassive Black Hole Growth

There is general consensus that active galactic nuclei (AGNs) derive their radiating power from a supermassive black hole (SMBH) that accretes matter. Yet, their precise powering mechanisms and the resulting growth of the SMBH are poorly understood, especially for AGNs at high redshift. Blazars are...

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Bibliographic Details
Main Authors: Jose Maria Sanchez Zaballa, Eugenio Bottacini, Andrea Tramacere
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Blazars
Flat-spectrum radio quasars
High-redshift galaxies
Supermassive black holes
Active galactic nuclei
Cosmological evolution
Online Access:https://doi.org/10.3847/1538-4357/adc994
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https://doi.org/10.3847/1538-4357/adc994

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