| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10694522 | Advances in Space Research | 2005 | 4 Pages |
Abstract
Preliminary results are presented from the CLEF hydrodynamics simulation, a large (N = 2 Ã 4283 particles within a 200 hâ1 Mpc comoving box) simulation of the ÎCDM cosmology that includes both radiative cooling and a simple model for galactic feedback. Specifically, we focus on the X-ray properties of the simulated clusters at z = 0 and demonstrate a reasonable level of agreement between simulated and observed cluster scaling relations.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
S.T. Kay, A.C. da Silva, N. Aghanim, A. Blanchard, A.R. Liddle, J.-L. Puget, R. Sadat, P.A. Thomas,