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Luminosity Function of Galaxies in Substructures of Galaxy Clusters

Published online by Cambridge University Press:  01 August 2006

Janusz Krywult
Janusz Krywult*
Affiliation:
Institute of Physics, Swietokrzyska Academy, Kielce, Poland email: krywult@pu.kielce.pl
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Abstract

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The analysis of the R-band luminosity function of galaxies in substructures of 21 Abell clusters shows that the characteristic magnitude M* for dominant substructure is brighter than in the second substructure and the magnitude gap between two brightest galaxies in dominant substructure is larger than in the second one.

Keywords

Galaxiesclustersluminosity functionsubstructures
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 217
Copyright
Copyright © International Astronomical Union 2007

References

Flin, P., & Krywult, J. 2006, AA 405, 9.CrossRefGoogle Scholar
Schechter, P. 1976, ApJ 203, 297.CrossRefGoogle Scholar