N-body Simulations of Galaxy Bars Generated by Satellite Collisions: Effects of the Impact Geometry
Bars, a common and important structure in disk galaxies, can be induced by galaxy interactions. Although there have been some studies on bar formation in flybys or collisions, the vast parameter space still leaves many scenarios that require further investigation. Here, we focus on the role of colli...
Saved in:
| Main Authors: | Yufan Fane Zhou, Zhiyuan Li, Hui Li |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/aded87 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The Abundance and Properties of Barred Galaxies out to z ∼ 4 Using JWST CEERS Data
by: Yuchen Guo, et al.
Published: (2025-01-01) -
Search for Slow Bars in Two Barred Galaxies with Nuclear Structures: NGC 6951 and NGC 7716
by: Yun Hee Lee, et al.
Published: (2025-01-01) -
Identification and Analysis of Galactic Bars in DESI Legacy Imaging Surveys
by: Wenwen Wang, 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) -
Comparison of Bar Formation Mechanisms. II. Does a Tidally Induced Bar Grow Faster than an Internally Developed Bar?
by: Yirui Zheng, et al.
Published: (2025-01-01)