Simulations of Milky Way-mass galaxies reveal direction-dependent dynamical heating during stellar radial migration, with inward migrators heating, some cooling, and cold preservation uncommon especially for older stars.
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N-body simulations show that subhaloes on low-inclination orbits to the galactic disc lose mass faster due to tidal shocks while exactly coplanar orbits experience suppressed mass loss from adiabatic shielding.
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Hot or Cold? Radial Redistribution of Stars in FIRE Simulations of Milky Way-Mass Galaxies and the Asymmetry of Inward versus Outward Migrators
Simulations of Milky Way-mass galaxies reveal direction-dependent dynamical heating during stellar radial migration, with inward migrators heating, some cooling, and cold preservation uncommon especially for older stars.
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Dynamical evolution of dark matter subhaloes in the Milky Way: role of the Galactic disc
N-body simulations show that subhaloes on low-inclination orbits to the galactic disc lose mass faster due to tidal shocks while exactly coplanar orbits experience suppressed mass loss from adiabatic shielding.