Clustering of faint galaxies

Details Clustering of faint galaxies Clustering of faint galaxies

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989rmxaa..19...71i&link_type=abstract

(Chile, una ventana de la astronomia optica; Coloquio, Santiago, Chile, Jan. 11-13, 1989) Revista Mexicana de Astronomia y Astro

Mathematics

Logic

Astronomical Catalogs, Faint Objects, Galactic Clusters, Galactic Structure, Statistical Analysis, Hubble Constant, Luminous Intensity, Power Spectra, Red Shift

Scientific paper

Research on the clustering of faint galaxies is reviewed, focusing on the evolution of clustering. Observational evidence supporting cosmological theories for the formation of the large-scale structure of the universe is discussed. The Gaussian and non-Gaussian models of universe and the statistical method used to study the large-scale structure are examined. Surveys of galaxies are listed and a new catalog of faint galaxies on a 3 x 3 deg area near the North Galactic Pole is described. It is found that the angular correlation function on small scales has a slope that is consistent with theoretical prediction (-0.8) and flattens toward fainter magnitudes.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1414691