The correlation function of galaxies in the direction of the Coma cluster

Details The correlation function of galaxies in the direction of the Coma cluster The correlation function of galaxies in the direction of the Coma cluster

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137..101c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 1, Oct. 1987, p. 101-106.

Astronomy and Astrophysics

Astrophysics

13

Data Correlation, Galactic Clusters, Data Sampling, Hubble Constant, Red Shift

Scientific paper

Data obtained by Einasto et al. (1986) on the amplitude of the correlation function of galaxies in the direction of the Coma cluster are compared with theoretical predictions of a model derived for a self-similar observer-homogeneous structure. The observational samples can be approximated by cones of angular width alpha of about 77 deg. Eliminating sources of large observational error, and by making a specified correction, the observational data are found to agree very well with the theoretical predictions of Calzetti et al. (1987).

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1773331