Dynamical friction in ultra-faint galaxies removes central dark matter via star-DM interactions, forming cores and compact stellar clusters with binaries.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
representative citing papers
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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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.