Dark matter profiles in clusters of galaxies: a phenomenological approach
- 31 August 2003
- journal article
- Published by Elsevier in New Astronomy
- Vol. 8 (6) , 517-528
- https://doi.org/10.1016/s1384-1076(03)00043-5
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This publication has 13 references indexed in Scilit:
- ChandraObservations of the Lensing Cluster EMSS 1358+6245: Implications for Self‐interacting Dark MatterThe Astrophysical Journal, 2002
- Deep inside the core of Abell 1795: theChandraviewMonthly Notices of the Royal Astronomical Society, 2002
- Dark Halos: The Flattening of the Density Cusp by Dynamical FrictionThe Astrophysical Journal, 2001
- A High‐Resolution Study of the Hydra A Cluster withChandra: Comparison of the Core Mass Distribution with Theoretical Predictions and Evidence for Feedback in the Cooling FlowThe Astrophysical Journal, 2001
- The Descendants of Lyman Break Galaxies in Galaxy Clusters: Spatial Distribution and Orbital PropertiesThe Astrophysical Journal, 2001
- The Density Profiles of the Dark Matter Halo Are Not UniversalThe Astrophysical Journal, 2000
- The gas fraction in clusters of galaxies as cosmological constraintAstronomische Nachrichten, 1999
- A Universal Density Profile from Hierarchical ClusteringThe Astrophysical Journal, 1997
- Simulations of X-ray clustersMonthly Notices of the Royal Astronomical Society, 1995
- Flow past a massive object and the gravitational dragThe Astrophysical Journal, 1980