Tracking the evolution of satellite galaxies: Mass stripping and dark-matter deficient galaxies
Date Issued
2024-01
Author(s) USM
DOI
10.1093/mnras/stad3268
Abstract
Satellite galaxies undergo a variety of physical processes when they are accreted by groups and clusters, often resulting in the loss of baryonic and dark matter (DM) mass. In this work, we evaluate the predictions from the Illustris TNG hydrodynamical si
