Observations and amr Simulations of the Evolution of Galaxy Clusters

Details Observations and amr Simulations of the Evolution of Galaxy Clusters Observations and amr Simulations of the Evolution of Galaxy Clusters

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.505b&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

We will present preliminary results from a numerical survey of galaxy groups and clusters using a new high spatial dynamic range, Eulerian, adapative mesh refinement, N-body/hydro code. The simulations were performed for an {Omega_o} + {Omegalambda} = 1 CDM Universe. We will discuss the evolution of the cluster mass, X-ray, and temperature functions, and will present initial results on the evolution of X-ray and temperature substructure, bulk flows, merger histories, and cooling flows. These numerical results will be compared with new ROSAT HRI, optical, and radio observations of z >= 0.2 Abell clusters and nearby poor clusters.

Affiliated with

Also associated with

No associations

Rating

Observations and amr Simulations of the Evolution of Galaxy 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 Observations and amr Simulations of the Evolution of Galaxy Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations and amr Simulations of the Evolution of Galaxy Clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-769765