Unraveling the Kinematic and Morphological Evolution of the Small Magellanic Cloud

Unraveling the Kinematic and Morphological Evolution of the Small Magellanic Cloud

We model the kinematics of the Small Magellanic Cloud (SMC) by analyzing the proper motions (PMs) from Gaia DR3 of nine different stellar populations, including young main-sequence (MS) stars (<2 Gyr), red giant branch stars, red clump stars, red giants with line-of-sight velocities, and three gr...

Full description

Saved in:
Bibliographic Details
Main Authors: S. R. Dhanush, A. Subramaniam, S. Subramanian
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Small Magellanic Cloud
Dwarf galaxies
Star clusters
Tidal interaction
Online Access:https://doi.org/10.3847/1538-4357/ada55f
Tags: Add Tag
No Tags, Be the first to tag this record!

Similar Items

Similar Items