BST1047+1156: A (Failing) Ultradiffuse Tidal Dwarf in the Leo I Group
We use deep Hubble Space Telescope imaging to study the resolved stellar populations in BST1047+1156, a gas-rich, ultradiffuse dwarf galaxy found in the intragroup environment of the Leo I galaxy group. While our imaging reaches approximately two magnitudes below the tip of the red giant branch at t...
Saved in:
Main Authors: | J. Christopher Mihos, Patrick R. Durrell, Aaron E. Watkins, Stacy S. McGaugh, John Feldmeier |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ad1cef |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Bullseye: HST, Keck/KCWI, and Dragonfly Characterization of a Giant Nine-ringed Galaxy
by: Imad Pasha, et al.
Published: (2025-01-01) -
Comparison of Bar Formation Mechanisms. I. Does a Tidally Induced Bar Rotate Slower than an Internally Induced Bar?
by: Yirui Zheng, et al.
Published: (2025-01-01) -
Introducing the Condor Array Telescope. V. Deep Broad- and Narrowband Imaging Observations of the M81 Group
by: Kenneth M. Lanzetta, et al.
Published: (2025-01-01) -
Investigating the Lower Limit of Metallicity for the Galactic Thin Disk
by: Guozhen Hu, et al.
Published: (2025-01-01) -
The Quest for a Stable Disk
by: J. A. Sellwood, et al.
Published: (2025-01-01)