An extended galaxy redshift survey. II - Virial constraints on Omega0. III - Constraints on large-scale structure

Mathematics – Logic

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Galactic Clusters, Galactic Mass, Red Shift, Virial Theorem, Astronomical Catalogs, Galactic Radiation, Luminosity, Mass Distribution, Virial Coefficients

Scientific paper

Results are presented from a cosmic virial theorem analysis of the 264 galaxies in the redshift survey of Metcalfe et al. (1989). Constraints on the cosmological density parameter, Omega0, are obtained. At scales less than 1/h Mpc, the mean mass density, Omega0 is estimated at 0.18 + or - 0.09. It is found that, at separation between about 2 and 7/h Mpc (H0 = 100 h km/s/Mpc) the redshift two-point correlation function, xi(s), has a correlation length of 7/h Mpc. At scales above 7/h Mpc, xi(s) breaks away quickly to zero. The results suggest that the universe is homogeneous to about 15 percent in Xi over scales up to 100/h Mpc.

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