The luminosity-diameter relationship of disk galaxies in clusters

Details The luminosity-diameter relationship of disk galaxies in clusters The luminosity-diameter relationship of disk galaxies in clusters

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...72..151g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 72, no. 1, Jan. 1988, p. 151-161. Research supported by the

Astronomy and Astrophysics

Astrophysics

8

Disk Galaxies, Galactic Clusters, Galactic Radiation, Galactic Structure, Galactic Evolution, Luminosity

Scientific paper

An examination of the absolute luminosities and sizes of ≡500 lenticular and spiral members of several clusters (Virgo, Hercules, Pegasus I, A262, A1367, A1656, Zwicky 74-23) has revealed appreciable differences in the galaxy luminosity-diameter relationships for different clusters. Discordances have emerged from a comparison with some earlier relevant investigations based on poorer statistics. Remarkably, the character of these relationships does not appear to depend on the presently observed main properties of clusters.

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