Correlation Functions from the Perseus-Pisces Redshift Survey

Details Correlation Functions from the Perseus-Pisces Redshift Survey Correlation Functions from the Perseus-Pisces Redshift Survey

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...419..451b&link_type=abstract

Astrophysical Journal v.419, p.451

Astronomy and Astrophysics

Astronomy

11

Galaxies: Clustering, Galaxies: Formation, Methods: Numerical

Scientific paper

The three- and four-point correlation functions are evaluated from the Perseus Pisces galaxy redshift sample. Former results on the two-point function ζ are also reviewed. In the range of distances from 1 h-1 Mpc to 10 h-1 Mpc, three- and four-point functions do not agree with the expressions of the hierarchical clustering model. On the contrary they are steeper and can be fitted by adding terms with a higher power of ζ. Such results from a redshift catalog partially modifies the picture of the large-scale matter distribution obtained from early two-dimensional samples. The relation among these results, biased models of galaxy formation, and observed velocity fields is discussed.

Affiliated with

Also associated with

No associations

Rating

Correlation Functions from the Perseus-Pisces Redshift Survey 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 Correlation Functions from the Perseus-Pisces Redshift Survey, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Correlation Functions from the Perseus-Pisces Redshift Survey will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-785071