Abstract
We use preliminary results of the WINGS survey (Fasano et al.) to obtain determinations of optical scaling relations for galaxy clusters. Passing from oneto twoparameter scaling relations we pay particular attention to the Kormendy relation (KR) and to the Fundamental Plane (FP) of galaxy clusters, comparing them with scaling relations of elliptical galaxies.
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Schedule a callMore From: Proceedings of the International Astronomical Union. International Astronomical Union
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