Simulating Chandra observations of galaxy clusters
Open Access
- 21 June 2004
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 351 (2) , 505-514
- https://doi.org/10.1111/j.1365-2966.2004.07800.x
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This publication has 45 references indexed in Scilit:
- X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulationMonthly Notices of the Royal Astronomical Society, 2004
- XMM‐NewtonObservations of the Perseus Cluster. I. The Temperature and Surface Brightness StructureThe Astrophysical Journal, 2003
- A Cold Front in a Preheated Galaxy ClusterThe Astrophysical Journal, 2002
- Evolution and structure of magnetic fields in simulated galaxy clustersAstronomy & Astrophysics, 2002
- Temperature Profiles of Nearby Clusters of GalaxiesThe Astrophysical Journal, 2002
- [ITAL]Chandra[/ITAL] Observation of the Radio Source/X-Ray Gas Interaction in the Cooling Flow Cluster Abell 2052The Astrophysical Journal, 2001
- Chandra imaging of the complex X-ray core of the Perseus clusterMonthly Notices of the Royal Astronomical Society, 2000
- The Evolution of X‐Ray Clusters in a Low‐Density UniverseThe Astrophysical Journal, 1998
- Mass Estimates of X-Ray ClustersThe Astrophysical Journal, 1996
- Parameter estimation in astronomy through application of the likelihood ratioThe Astrophysical Journal, 1979