First Observation of a Double-peaked O i Emission in the Near-infrared Spectrum of an Active Galaxy

Double-peaked profiles associated with the broad-line region (BLR) of active galactic nuclei (AGNs) are regarded as the clearest evidence of the presence of an accretion disk. They are most commonly detected by means of optical spectroscopy in the Balmer lines and in the Mg ii λ 2798 ultraviolet lin...

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Bibliographic Details
Main Authors: Denimara Dias dos Santos, Alberto Rodríguez-Ardila, Swayamtrupta Panda, Murilo Marinello
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/ace974