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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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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