Low mass portion of the galaxy clustering spectrum

Details Low mass portion of the galaxy clustering spectrum Low mass portion of the galaxy clustering spectrum

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.274..450g&link_type=abstract

Nature, vol. 274, Aug. 3, 1978, p. 450-452.

Computer Science

5

Galactic Clusters, Mass Distribution, Red Shift, Spectrum Analysis, Galactic Radiation, Line Spectra, Luminous Intensity, Power Spectra, Space Density, Stellar Mass

Scientific paper

A log distribution is presented to illustrate the clustering spectrum of galaxies and groups of galaxies investigated by a complete redshift survey. Attention is given to the low-mass portion of the clustering spectrum for eight groups of galactic clouds which lie in the 42,000 cubic Mpc region between the Local and the Coma/A1367 superclusters (assuming the traditional value for H). It is noted that only four galaxies of the eight galactic groups surveyed can be considered as isolated, and it is suggested that single galaxies are merely the faint end of the cluster luminosity spectrum.

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