Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-16T15:27:27.823Z Has data issue: false hasContentIssue false
  • English
  • Français

Luminosity Distribution in CD Clusters

Published online by Cambridge University Press:  26 July 2016

F.W. Baier
F.W. Baier*
Affiliation:
WIP - Working Group ‘Galaxy Clusters’, University of Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The ratio of contributions from cannibalism and from cooling flows to the final cD galaxies in diverse clusters seems to be different. It should be determined by some general cluster properties as for instance the central mass concentration. Assuming that mass distribution is tantamount to luminosity distribution we have analyzed the question of possible luminosity segregation in the radial galaxy distribution of galaxy clusters (Baier & Schmidt 1992; Baier & MacGillivray 1994).

Type
Part Thirteen: Properties and Clustering of Galaxies and Clusters
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 629 - 631
Copyright
Copyright © Kluwer 1994 

References

Baier, F.W. and Schmidt, K.-H., 1992. Astron. Nachr., 313, 275.Google Scholar
Baier, F.W. and MacGillivray, H.T., 1994. Mon. Not. R. astron. Soc., in preparation.Google Scholar
Bhavsar, S.P., 1989. Astrophys. J., 338, 718.Google Scholar
Bothun, G.D. and Schombert, J.M., 1990. Astrophys. J., 360, 436.CrossRefGoogle Scholar
Gudehus, D.H., 1991. Astrophys. J., 382, 1.Google Scholar
Lugger, P.M., 1984. Astrophys. J., 278, 51.Google Scholar
Lugger, P.M., 1989. Astrophys. J., 343, 572.CrossRefGoogle Scholar
Malumuth, E.M., 1992. Astrophys. J., 386, 420.Google Scholar
Porter, A.C., 1988. PhD Thesis, Caltech.Google Scholar
Porter, A.C., Schneider, D.P. and Hoessel, J.G., 1991. Astron. J., 101, 1561.CrossRefGoogle Scholar