Simulating Intermediate Black Hole Mass Measurements for a Sample of Galaxies with Nuclear Star Clusters Using ELT/HARMONI High Spatial Resolution Integral-field Stellar Kinematics

Simulating Intermediate Black Hole Mass Measurements for a Sample of Galaxies with Nuclear Star Clusters Using ELT/HARMONI High Spatial Resolution Integral-field Stellar Kinematics

Understanding the demographics of intermediate-mass black holes (IMBHs, M _BH  ≈ 10 ^2 –10 ^5 M _⊙ ) in low-mass galaxies is key to constraining black hole seed formation models, but detecting them is challenging due to their small gravitational sphere of influence (SOI). The upcoming Extremely Larg...

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Bibliographic Details
Main Authors: Dieu D. Nguyen, Michele Cappellari, Hai N. Ngo, Tinh Q. T. Le, Tuan N. Le, Khue N. H. Ho, An K. Nguyen, Phong T. On, Huy G. Tong, Niranjan Thatte, Miguel Pereira-Santaella
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
Subjects:
Astrophysical black holes
Galaxy kinematics
Galaxy dynamics
Galaxy nuclei
Galaxy spectroscopy
Astronomy data modeling
Online Access:https://doi.org/10.3847/1538-3881/ade9ba
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https://doi.org/10.3847/1538-3881/ade9ba

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