In the MTNG simulation, satellite galaxies lose ~80% of their gas by the time their subhalos lose half their mass, while stellar mass and magnitudes evolve more slowly following v_max reduction, with inner mass loss occurring early.
We find that, by using the same pa- rameterisation as forv max/vinfall, we can recover the evolution of most properties almost perfectly
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The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations
In the MTNG simulation, satellite galaxies lose ~80% of their gas by the time their subhalos lose half their mass, while stellar mass and magnitudes evolve more slowly following v_max reduction, with inner mass loss occurring early.