• Yang-Shyang Li
  • YAmina Helmi
Part of the Astrophysics and Space Science Proceedings book series (ASSSP)


We analyze properties of subhalos/substructures resolved in a dark matter simulation of a Milky Way-like halo in a ΛCDM cosmology. We explore possible links between subhalos and the Galactic satellites and find: 1) The infall patterns of subhalos are slightly elongated along the major axis of the galaxy halo and are clumpy on smaller scales. 2) The Great disk defined by MW satellites (Kroupa et al. 2005) is easily reproduced in our simulations without recurring to sophisticated galaxy formation recipes and is purely due to their highly centrally concentrated distribution around the Galaxy.


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Copyright information

© Springer 2007

Authors and Affiliations

  • Yang-Shyang Li
    • 1
  • YAmina Helmi
    • 1
  1. 1.Kapteyn Astronomical InstituteUniversity of GroningenThe Netherlands

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