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The reliability of the kinematical evidence for dark matter: the effects of non-sphericity, substructure and streaming motions
Authors:Teresa Sanchis  Ewa L &#;okas  Gary A Mamon
Institution:Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Avenida Diagonal 647, E-08028 Barcelona, Spain;Nicolaus Copernicus Astronomical Centre, Bartycka 18, 00-716 Warsaw, Poland;Institut d'Astrophysique de Paris (CNRS UMR 7095), 98 bis Bd Arago, F-75014 Paris, France;GEPI (CNRS UMR 8111), Observatoire de Paris, F-92195 Meudon, France
Abstract:
Keywords:methods: analytical  methods: N-body simulations  galaxies: clusters: general  galaxies: kinematics and dynamics  dark matter
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