Finding Massive Double-exponential Disk Galaxies with Extended Low Surface Brightness Stellar Disk: An IllustrisTNG Exploration
We study massive disk galaxies (stellar mass > = 10 ^11 M _⊙ ) at z = 0 from IllustrisTNG simulation to detect galaxies that contain two exponential stellar disks—a central high surface brightness (HSB) disk surrounded by an extended low surface brightness (LSB) envelope. This is motivated by the...
Saved in:
| Main Authors: | Suchira Sarkar, Kanak Saha |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adcea5 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
by: Yingzhong Xu, et al.
Published: (2022-01-01) -
Enhanced Star Formation and Black Hole Accretion Rates in Galaxy Mergers in IllustrisTNG50
by: Aimee L. Schechter, et al.
Published: (2025-01-01) -
The Intrinsic Flattening of Galaxy Disks
by: Jeremy Favaro, et al.
Published: (2024-01-01) -
Mass growth of massive quiescent galaxies in the Illustris TNG simulation
by: Bendegúz Koncz, et al.
Published: (2025-03-01) -
Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
by: Kun Xu, et al.
Published: (2025-01-01)