Structure and formation of superclusters. VII - Distribution of bright and faint galaxies in the Virgo supercluster

Details Structure and formation of superclusters. VII - Distribution of bright and faint galaxies in the Virgo supercluster Structure and formation of superclusters. VII - Distribution of bright and faint galaxies in the Virgo supercluster

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234...37e&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Sept. 1, 1988, p. 37-50.

Astronomy and Astrophysics

Astronomy

17

Brightness Distribution, Faint Objects, Galactic Structure, Virgo Galactic Cluster, Dark Matter, Dwarf Galaxies, Spatial Distribution

Scientific paper

The spatial distributions of bright and faint galaxies in the Virgo supercluster are compared using the nearest neighbour test and cluster analysis. There are no differences in the spatial distribution of bright and faint galaxies down to the absolute magnitude -15.0 (H = 100 km s-1Mpc-1). Bright and faint galaxies are situated in statistically identical systems, and the ratio of faint/bright galaxies is nearly the same in high- and low-density regions.

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