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Multiple merging in the Abell cluster 1367
Published online by Cambridge University Press: 06 October 2004
Abstract
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