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Why the Canis Major overdensity is not due to the Warp: analysis of its radial profile and velocities
Authors:N F Martin  R A Ibata  B C Conn  G F Lewis  M Bellazzini  M J Irwin  A W McConnachie
Institution:Observatoire de Strasbourg, 11 rue de l'Université, F-67000 Strasbourg, France;Institute of Astronomy, School of Physics, A29, University of Sydney, NSW 2006, Australia;INAF –Osservatorio Astronomico di Bologna, Via Ranzani 1, 40127 Bologna, Italy;Institute of Astronomy, Madingley Road, Cambridge CB3 0HA
Abstract:
Keywords:Galaxy: formation  Galaxy: structure  galaxies: interactions
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