Tidal debris of dwarf spheroidals as a probe of structure formation models
Open Access
- 11 October 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 336 (1) , 119-130
- https://doi.org/10.1046/j.1365-8711.2002.05721.x
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This publication has 83 references indexed in Scilit:
- Halo Cores and Phase‐Space Densities: Observational Constraints on Dark Matter Physics and Structure FormationThe Astrophysical Journal, 2001
- Formation and Structure of Halos in a Warm Dark Matter CosmologyThe Astrophysical Journal, 2001
- Constraints on Warm Dark Matter from Cosmological ReionizationThe Astrophysical Journal, 2001
- Interpreting Debris from Satellite Disruption in External GalaxiesThe Astrophysical Journal, 2001
- Stars of the Draco Dwarf Spheroidal Galaxy Beyond Its Measured Tidal BoundaryThe Astronomical Journal, 2001
- Mapping the Galactic Halo. IV. Finding Distant Giants Reliably with the Washington SystemThe Astronomical Journal, 2001
- Weakly Self-interacting Dark Matter and the Structure of Dark HalosThe Astrophysical Journal, 2000
- Dwarf spheroidal satellite galaxies without dark matterNew Astronomy, 1997
- Unbound dwarf spheroidal galaxies and the mass of the Milky WayThe Astrophysical Journal, 1993
- Dark halos formed via dissipationless collapse. I - Shapes and alignment of angular momentumThe Astrophysical Journal, 1992