A 22 Billion M⊙ Black Hole in Holmberg 15A with Keck KCWI Spectroscopy and Triaxial Orbit Modeling
Holmberg 15A (H15A), the brightest cluster galaxy of A85, has an exceptionally low central surface brightness even among local massive elliptical galaxies with distinct stellar cores, making it exceedingly challenging to obtain high-quality spectroscopy to detect a supermassive black hole (SMBH) at...
Saved in:
| Main Authors: | Emily R. Liepold, Chung-Pei Ma, Jonelle L. Walsh |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ada4b0 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The MASSIVE Survey. XX. A Triaxial Stellar Dynamical Measurement of the Supermassive Black Hole Mass and Intrinsic Galaxy Shape of Giant Radio Galaxy NGC 315
by: Jacob Pilawa, et al.
Published: (2025-01-01) -
From Halos to Galaxies. VI. Improved Halo Mass Estimation for SDSS Groups and Measurement of the Halo Mass Function
by: Dingyi Zhao, et al.
Published: (2025-01-01) -
The RESOLVE and ECO Gas in Galaxy Groups Initiative: The Group Finder and the Group H i–Halo Mass Relation
by: Zackary L. Hutchens, et al.
Published: (2023-01-01) -
The Impact of Applying Black Hole–Host Galaxy Scaling Relations to Large Galaxy Populations
by: Maggie C. Huber, et al.
Published: (2025-01-01) -
The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
by: Zhenjie Liu, et al.
Published: (2025-01-01)