SIDM simulations of dwarf halos show that quiescent merger histories produce gravothermal core collapse while sustained mergers prevent collapse and can yield central densities below gravothermal fluid model predictions.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
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2026 3verdicts
UNVERDICTED 3representative citing papers
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.
New SBF distance confirms NGC5846_UDG1 lies in the NGC 5846 group and reconciles prior GC counts to ~50 members, supporting a massive dark matter halo.
citing papers explorer
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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.