Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-11-07
Astronomy and Astrophysics
Astrophysics
4 pages, 1 figure, contribution to "Tracing cosmic evolution with galaxy clusters" (Sesto 2001), ASP Conference Series
Scientific paper
The results from hydrodynamical TREESPH simulations of galaxy clusters are used to investigate the dependence of the final cluster X-ray properties upon the numerical resolution and the assumed star formation models for the cooled gas. When cold gas particles are allowed to convert into stars the final gas profiles show a well defined core radius and the temperature profiles are nearly flat. Final X-ray luminosities are found to be numerically stable, with uncertainties of a factor 2.
No associations
LandOfFree
Radiative cooling in SPH hydrodynamical simulations of X-ray clusters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radiative cooling in SPH hydrodynamical simulations of X-ray clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative cooling in SPH hydrodynamical simulations of X-ray clusters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-102258