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Subclustering in Cooling and Non-cooling Flow Clusters
Published online by Cambridge University Press: 26 May 2016
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
References
Escalera, E., Biviano, A., Girardi, M., Mardirossian, F., Mazure, A., Mezzetti, M., 1994, ApJ
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