Simulations find that tidal dwarf galaxies form and persist in galaxy clusters under moderate stellar feedback across all relevant viscosities, supporting their identification as stripped remnants matching multiple observed dwarf galaxy classes.
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A switch-free artificial viscosity scheme in SPH using velocity reconstruction and Balsara correction achieves balanced dissipation and lower spurious noise than traditional switch-based methods.
citing papers explorer
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Merge and Strip II: Imprint of galaxy formation physics and viscosity on baryon-dominated dwarf galaxies
Simulations find that tidal dwarf galaxies form and persist in galaxy clusters under moderate stellar feedback across all relevant viscosities, supporting their identification as stripped remnants matching multiple observed dwarf galaxy classes.
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Are heuristic switches necessary to control dissipation in modern smoothed particle hydrodynamics ?
A switch-free artificial viscosity scheme in SPH using velocity reconstruction and Balsara correction achieves balanced dissipation and lower spurious noise than traditional switch-based methods.