Comparing galactic satellite properties in hydrodynamical and N-body simulations

@article{Schewtschenko2010ComparingGS,
  title={Comparing galactic satellite properties in hydrodynamical and N-body simulations},
  author={Jascha A. Schewtschenko and Andrea V. Macci{\`o}},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2010},
  volume={413},
  pages={878-886}
}
In this work, we examine the different properties of galactic satellites in hydrodynamical and pure dark matter simulations. We use three pairs of simulations (collisional and collisionless) starting from identical initial conditions. We concentrate our analysis on pairs of satellites in the hydro and N-body runs that form from the same Lagrangian region. We look at the radial positions, mass-loss as a function of time and orbital parameters of these ‘twin’ satellites. We confirm an overall… Expand
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