Dynamical friction in ultra-faint galaxies removes central dark matter via star-DM interactions, forming cores and compact stellar clusters with binaries.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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High-resolution SPH simulations show that significant in-plane spreading and dissipation of returning tidal debris at pericenter is a low-resolution numerical artifact, supporting circularization via later stream-stream collisions instead.
SPH simulations show that ice can be preferentially stripped from a differentiated moon during close encounters with Saturn to produce rings matching the observed mass and composition, if the closest approach lies between the ice and rock Roche limits.
citing papers explorer
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Collisional Dynamics of Stars and Dark Matter in Ultra-Faint Galaxies
Dynamical friction in ultra-faint galaxies removes central dark matter via star-DM interactions, forming cores and compact stellar clusters with binaries.
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Tidal disruption events with SPH-EXA: resolving the return of the stream
High-resolution SPH simulations show that significant in-plane spreading and dissipation of returning tidal debris at pericenter is a low-resolution numerical artifact, supporting circularization via later stream-stream collisions instead.
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Investigating tidal stripping of a pre-existing moon as the origin of Saturn's young icy rings
SPH simulations show that ice can be preferentially stripped from a differentiated moon during close encounters with Saturn to produce rings matching the observed mass and composition, if the closest approach lies between the ice and rock Roche limits.