Galaxy Clustering Morphology and Luminosity

Details Galaxy Clustering Morphology and Luminosity Galaxy Clustering Morphology and Luminosity

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.265...21i&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 265, NO. 1/NOV1, P. 21, 1993

Mathematics

Logic

44

Scientific paper

The aim of this paper is to study the space distribution of galaxies with a view to determining whether the known morphology-density and luminosity-density relationships are unrelated or are a consequence of different luminosity functions for different morphological types. It is found that morphology and luminosity are two independent parameters that affect both the clustering properties of galaxies and their distribution as a function of the local density, morphology playing the predominant role.

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