Simulating the physical properties of dark matter and gas inside the cosmic web
Open Access
- 22 June 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 370 (2) , 656-672
- https://doi.org/10.1111/j.1365-2966.2006.10511.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 72 references indexed in Scilit:
- The Fall of Active Galactic Nuclei and the Rise of Star-forming Galaxies: A Close Look at the Chandra Deep Field X-Ray Number CountsThe Astronomical Journal, 2004
- Using the Filaments in the Las Campanas Redshift Survey to Test the ΛCDM ModelThe Astrophysical Journal, 2004
- Cosmic Filaments in SuperclustersThe Astrophysical Journal, 2004
- X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulationMonthly Notices of the Royal Astronomical Society, 2004
- The X‐Ray Surface Brightness Distribution from Diffuse GasThe Astrophysical Journal, 2001
- The [ITAL]CHANDRA[/ITAL][ITAL]Chandra[/ITAL] Deep Survey of the Hubble Deep Field North Area. IV. An Ultradeep Image of the HDF-NThe Astronomical Journal, 2001
- A study of the core of the Shapley Concentration -- IV. Distribution of intercluster galaxies and supercluster propertiesMonthly Notices of the Royal Astronomical Society, 2000
- Where Are the Baryons?The Astrophysical Journal, 1999
- Statistical Properties of X‐Ray Clusters: Analytic and Numerical ComparisonsThe Astrophysical Journal, 1998
- How filaments of galaxies are woven into the cosmic webNature, 1996