The influence of large-scale structures on halo shapes and alignments
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Open Access
- 21 June 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 370 (3) , 1422-1428
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This publication has 42 references indexed in Scilit:
- The Orientation of Satellite Galaxies: Evidence of Elongation in the Direction of the HostThe Astrophysical Journal, 2006
- The shape of dark matter haloes: dependence on mass, redshift, radius and formationMonthly Notices of the Royal Astronomical Society, 2006
- The shape-alignment relation in cold dark matter cosmic structuresMonthly Notices of the Royal Astronomical Society, 2006
- Intercluster filaments in a CDM UniverseMonthly Notices of the Royal Astronomical Society, 2005
- Figure Rotation of Cosmological Dark Matter HalosThe Astrophysical Journal, 2004
- The Nearest Neighbor Alignment of Cluster X‐Ray IsophotesThe Astrophysical Journal, 2002
- Weak‐Lensing Surveys and the Intrinsic Correlation of Galaxy EllipticitiesThe Astrophysical Journal, 2000
- EinsteinCluster Alignments RevisitedThe Astrophysical Journal, 2000
- Linking cluster formation to large-scale structureMonthly Notices of the Royal Astronomical Society, 1999
- How filaments of galaxies are woven into the cosmic webNature, 1996