Uncovering cold dark matter halo substructure with tidal streams
Open Access
- 1 June 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 332 (4) , 915-920
- https://doi.org/10.1046/j.1365-8711.2002.05358.x
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This publication has 29 references indexed in Scilit:
- Probing Dark Matter Substructure in Lens GalaxiesThe Astrophysical Journal, 2002
- GAIA: Composition, formation and evolution of the GalaxyAstronomy & Astrophysics, 2001
- Structure of the Galactic Stellar Halo Prior to Disk FormationThe Astrophysical Journal, 2001
- Detection of Massive Tidal Tails around the Globular Cluster Palomar 5 with Sloan Digital Sky Survey Commissioning DataThe Astrophysical Journal, 2001
- High‐Velocity Clouds: Building Blocks of the Local GroupThe Astrophysical Journal, 1999
- Destruction of the Galactic Globular Cluster SystemThe Astrophysical Journal, 1997
- Globular Clusters with Tidal Tails: Deep Two-Color Star CountsThe Astronomical Journal, 1995
- The effect of dissipation on the shapes of dark halosThe Astrophysical Journal, 1994
- Dark halos formed via dissipationless collapse. I - Shapes and alignment of angular momentumThe Astrophysical Journal, 1992
- Dissipationless collapse in an expanding universeThe Astrophysical Journal, 1991