Correlation functions of galaxies with different weightings according to luminosity and mass

Details Correlation functions of galaxies with different weightings according to luminosity and mass Correlation functions of galaxies with different weightings according to luminosity and mass

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...221..191b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 221, no. 2, Sept. 1989, p. 191-196.

Astronomy and Astrophysics

Astrophysics

27

Galactic Clusters, Galactic Mass, Luminosity, Correlation, Mass To Light Ratios

Scientific paper

Two-point correlation functions of galaxies with luminosity-weighting and mass-weighting are studied to determine the dependence of the clustering properties on the intrinsic properties of galaxies. The results suggest that bright galaxies with M(B) of less than -20.5 and early stage galaxies tend to be more correlated on scales of less than 14 Mpc (h = 1/2). The brightest galaxies and Sb-SC galaxies are shown to be preferentially distributed with separations of about 9 Mpc. A power law dependence of the correlation length on the limiting luminosity of the sample is found.

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