Photometry of the rich cluster of galaxies 0004.8-3450

Details Photometry of the rich cluster of galaxies 0004.8-3450 Photometry of the rich cluster of galaxies 0004.8-3450

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.190..307c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 190, Jan. 1980, p. 307-320.

Other

32

Astronomical Photography, Astronomical Photometry, Galactic Clusters, Galactic Structure, Brightness, Energy Distribution, Luminosity, Red Shift, Spiral Galaxies

Scientific paper

Photographic photometry of the rich cluster of galaxies 0004.8-3450 is presented. The cluster is centered on an unusually elongated cD galaxy; the luminosity function for 1552 galaxies shows a form more characteristic of loose clusters with some spirals than of clusters with cD galaxies. The distributions of very red and blue galaxies do not show that they are cluster members; there is some evidence for a deficiency of other elongated galaxies with the same position angle as the cD.

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