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Multiple merging in the Abell cluster 1367

Published online by Cambridge University Press:  06 October 2004

L. Cortese ,
G. Gavazzi  and
A. Boselli
L. Cortese
Affiliation:
Università degli Studi di Milano-Bicocca, P.zza della Scienza 3, 20126 Milano, Italy email: Luca.Cortese@mib.infn.it; Giuseppe.Gavazzi@mib.infn.it
G. Gavazzi
Affiliation:
Università degli Studi di Milano-Bicocca, P.zza della Scienza 3, 20126 Milano, Italy email: Luca.Cortese@mib.infn.it; Giuseppe.Gavazzi@mib.infn.it
A. Boselli
Affiliation:
Laboratoire d'Astrophysique de Marseille, BP8, Traverse du Siphon, F-13376 Marseille, France email: alessandro.boselli@oamp.fr
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Abstract

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We present a dynamical analysis of the central $\sim$ 1.3 square degrees of the galaxy cluster Abell 1367, based on 272 redshift (of which 118 are new measurements). From the analysis of the 146 confirmed cluster members Abell 1367 appears as a young cluster currently forming at the intersection of two filaments.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. 92 - 94
Copyright
© 2004 International Astronomical Union