There is strong evidence that the mass of the Universe is dominated by dark matter, which exerts gravitational attraction but whose exact nature is unknown. In particular, all galaxies are believed to be embedded in massive haloes of dark matter^{1, 2}. This view has recently been challenged by the observation of surprisingly low random stellar velocities in the outskirts of ordinary elliptical galaxies, which has been interpreted as indicating a lack of dark matter^{3, 4}. Here we show that the low velocities are in fact compatible with galaxy formation in dark-matter haloes. Using numerical simulations of disk-galaxy mergers^{5, 6}, we find that the stellar orbits in the outer regions of the resulting ellipticals are very elongated. These stars were torn by tidal forces from their original galaxies during the first close passage and put on outgoing trajectories. The elongated orbits, combined with the steeply falling density profile of the observed tracers, explain the observed low velocities even in the presence of large amounts of dark matter. Projection effects when viewing a triaxial elliptical can lead to even lower observed velocities along certain lines of sight.

1. Racah Institute of Physics, The Hebrew University, Jerusalem 91904, Israel
2. Institut d'Astrophysique, 98bis Boulevard Arago, Paris 75014, France
3. Observatoire de Paris, F-92195 Meudon, France
4. Department of Physics,
5. UCO/Lick Observatories, University of California, Santa Cruz, California 95064, USA
6. Center for Astrophysics, Harvard University, 60 Garden Street, Cambridge, Massachusetts 02138, USA

Correspondence to: A. Dekel^1,2,3,4 Correspondence and requests for materials should be addressed to A.D. (Email: dekel@phys.huji.ac.il).

Received 27 January 2005; Accepted 22 June 2005

MORE ARTICLES LIKE THIS

These links to content published by NPG are automatically generated.