A Dual Active Black Hole Candidate with Mass Ratio ~7:1 in a Disk Galaxy

A Dual Active Black Hole Candidate with Mass Ratio ~7:1 in a Disk Galaxy

Dual active galactic nuclei (AGNs) with comparable masses are commonly witnessed among the major merged galaxies with interaction remnants. Considering almost every massive galaxy is associated with multiple dwarf satellites around it, minor mergers involving galaxies with disproportional stellar ma...

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Bibliographic Details
Main Authors: Xiao Cao, Yan-Mei Chen, Yong Shi, Junfeng Wang, Zhijie Zhou, Min Bao, Qiusheng Gu, Alexei Moiseev, Luis C. Ho, Lan Wang, Guangquan Zeng
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Galaxy kinematics
Galactic winds
Galaxy evolution
Online Access:https://doi.org/10.3847/2041-8213/adaa7b
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https://doi.org/10.3847/2041-8213/adaa7b

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