Core Structure of Intracluster Gas: Isothermal Hydrostatic Equilibrium
- 25 June 2005
- journal article
- Published by Oxford University Press (OUP) in Publications of the Astronomical Society of Japan
- Vol. 57 (3) , 419-427
- https://doi.org/10.1093/pasj/57.3.419
Abstract
No abstract availableAll Related Versions
This publication has 32 references indexed in Scilit:
- X-ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulationMonthly Notices of the Royal Astronomical Society, 2004
- The new emerging model for the structure of cooling cores in clusters of galaxiesAstronomy & Astrophysics, 2002
- Details of the mass-temperature relation for clusters of galaxiesAstronomy & Astrophysics, 2001
- The WARPS survey - IV. The X-ray luminosity-temperature relation of high-redshift galaxy clustersMonthly Notices of the Royal Astronomical Society, 2000
- The LX--T relation and intracluster gas fractions of X-ray clustersMonthly Notices of the Royal Astronomical Society, 1999
- Quantifying the Morphologies and Dynamical Evolution of Galaxy Clusters. II. Application to a Sample of ROSAT ClustersThe Astrophysical Journal, 1996
- Cooling Flows in Clusters of GalaxiesAnnual Review of Astronomy and Astrophysics, 1994
- TREESPH - A unification of SPH with the hierarchical tree methodThe Astrophysical Journal Supplement Series, 1989
- Solid Polyomino ConstructionsMathematics Magazine, 1976
- On the Classification of the Forms of Clusters of GalaxiesThe Astrophysical Journal, 1970