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Subclustering in Cooling and Non-cooling Flow Clusters

Published online by Cambridge University Press:  26 May 2016

P. Flin  and
J. Krywult
P. Flin
Affiliation:
Pedagogical University, Institute of Physics, ul. Swietokrzyska 15, 25-406 Kielce, Poland Joint Institute for Nuclear Research, Bogoliubov Laboratory of Theoretical Physics, Dubna, Moscow Region 141 980, Russia
J. Krywult
Affiliation:
Pedagogical University, Institute of Physics, ul. Swietokrzyska 15, 25-406 Kielce, Poland

Abstract

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For 20 hot luminous Beppo-SAX galaxy clusters the occurrence of substrucures has been investigated in 2-D optical data, mainly through the application of the wavelet analysis. Our results are compared with others, coming from 3-D optical data, as well as X-rays. In this sample of galaxy clusters a higher percentage of substructure is observed among non-cooling flow clusters than cooling flow clusters.

Type
Part 1. Census
Information
Symposium - International Astronomical Union , Volume 217: Recycling Intergalactic and Interslettar Matter , 2004 , pp. 118 - 120
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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