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Scaling relations for galaxy clusters

Published online by Cambridge University Press:  06 October 2004

C. Marmo ,
G. Fasano ,
E. Pignatelli ,
B. Poggianti ,
D. Bettoni ,
C. Halliday ,
J. Varela ,
M. Moles ,
P. Kjærgaard  and
W. Couch
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C. Marmo
Affiliation:
Astronomy Department, University of Padova, Italy email: marmo@pd.astro.it
G. Fasano
Affiliation:
INAF, Osservatorio Astronomico di Padova, Italy
E. Pignatelli
Affiliation:
INAF, Osservatorio Astronomico di Padova, Italy
B. Poggianti
Affiliation:
INAF, Osservatorio Astronomico di Padova, Italy
D. Bettoni
Affiliation:
INAF, Osservatorio Astronomico di Padova, Italy
C. Halliday
Affiliation:
INAF, Osservatorio Astronomico di Padova, Italy
J. Varela
Affiliation:
IMAFF, CSIC, Madrid, Spain
M. Moles
Affiliation:
Instituto de Astrofísica de Andalucía, Granada, Spain
P. Kjærgaard
Affiliation:
Copenhagen University Observatory, Copenhagen, Denmark
W. Couch
Affiliation:
School of Physics, University of New South Wales, Sydney, Australia
A. Dressler
Affiliation:
Observatories of the Carnegie Institution of Washington, Pasadena, USA
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Abstract

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We use preliminary results of WINGS survey (Fasano et al.) to obtain determinations of optical scaling relations for galaxy clusters. Passing from one- to two- parameter 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.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 242 - 244
Copyright
© 2004 International Astronomical Union