On the Significance of the Thick Disks of Disk Galaxies
Thick disks are a prevalent feature observed in numerous disk galaxies, including our own Milky Way. Their significance has been reported to vary widely, ranging from a few percent to 100% of the disk mass, depending on the galaxy and the measurement method. We use the NewHorizon simulation, which h...
Main Authors: | Sukyoung K. Yi, J. K. Jang, Julien Devriendt, Yohan Dubois, San Han, Taysun Kimm, Katarina Kraljic, Minjung Park, Sebastien Peirani, Christophe Pichon, Jinsu Rhee |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
|
Series: | The Astrophysical Journal Supplement Series |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4365/ad0e71 |
Similar Items
-
Probing the History of the Galaxy Assembly of the Counterrotating Disk Galaxy PGC 66551
by: Ivan Yu. Katkov, et al.
Published: (2024-01-01) -
The Thickness of Galaxy Disks from z = 5 to 0 Probed by JWST
by: Jianhui Lian, et al.
Published: (2024-01-01) -
Effects of the Central Mass Concentration on Bar Formation in Disk Galaxies
by: Dajeong Jang, et al.
Published: (2023-01-01) -
Resolved SPLASH Chemodynamics in Andromeda’s PHAT Stellar Halo and Disk: On the Nature of the Inner Halo along the Major Axis
by: Ivanna Escala, et al.
Published: (2023-01-01) -
Properties of Stellar Streams in the Galactic Disk
by: Marsakov V. A., et al.
Published: (2016-12-01)