The spatial correlation function of superclusters of galaxies

Details The spatial correlation function of superclusters of galaxies The spatial correlation function of superclusters of galaxies

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14...18l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Jan. 1988, p. 18-22. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

5

Galactic Clusters, Galactic Structure, Space Density, Statistical Correlation, Gamma Ray Astronomy, Series (Mathematics)

Scientific paper

The two-point correlation function was computed for 49 superclusters of galaxies localized in the region with a galactic latitude greater than 30 deg. On scales of 100-400 Mpc (H = 75 km/s/Mpc), the correlation function is described by a power law (r/r0) exp -gamma, where gamma = 1.8 + or - 0.2 and r0 = 120 + or - 20 Mpc. The spatial density of superclusters is analyzed as a function of distance.

Affiliated with

Also associated with

No associations

Rating

The spatial correlation function of superclusters of galaxies 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 spatial correlation function of superclusters of galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spatial correlation function of superclusters of galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1049062