2004/02/01 by A. Da Silva, Antonio C. da Silva
Physics and Astronomy · #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Scientific Research and Discoveries #astro-ph
paper · pdf · doi:10.1023/b:astr.0000022172.80206.d6
published as Astrophys.Space Sci. 290 (2004) 167-176 · 10 pages, 3 figures, LaTeX. To appear in proceedings of the JENAM 2002 conference. For a more detailed analysis see astro-ph/0308074, whose simulations supersede those presented at this conference
openalex publication_date 2004/02/01 · arxiv created 2004/03/23 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Observations with the SZ effect constitute a powerful new tool for investigating clusters and constraining cosmological parameters. Of particular interest is to investigate how the SZ signal correlates with other cluster properties, such as the mass, temperature and X-ray luminosities. In this presentation we quantify these relations for clusters found in hydrodynamical simulations of large scale structure and investigate their dependence on the effects of radiative cooling and pre-heating.