The cluster-cluster correlation in hybrid models

Details The cluster-cluster correlation in hybrid models The cluster-cluster correlation in hybrid models

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...411..450j&link_type=abstract

Astrophysical Journal - Part 1 (ISSN 0004-637X), vol. 411, no. 2, p. 450-454.

Astronomy and Astrophysics

Astrophysics

28

Angular Correlation, Astronomical Models, Dark Matter, Galactic Clusters, Interacting Galaxies, Many Body Problem, Galactic Evolution, Galactic Structure, Universe

Scientific paper

N-body simulations are here used to calculate the two-point correlation functions (TPCFs) of galaxy clusters in a set of cold dark matter/hot dark matter/baryon-containing hybrid models. The clusters of galaxies are identified so that their number density is the same as that of Abell clusters. Both the coherence length and the amplitude of the TPCFs systematically increase with the power of the initial density spectrum on large scales. These results suggest that the observed large correlation length of Abell clusters should be expected in models with enough power to explain galaxy clustering and large scale motions.

Affiliated with

Also associated with

No associations

Rating

The cluster-cluster correlation in hybrid models 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 The cluster-cluster correlation in hybrid models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The cluster-cluster correlation in hybrid models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1069272