Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-25T18:38:59.308Z Has data issue: false hasContentIssue false
  • English
  • Français

Wide-field spectroscopy of a galaxy cluster pair at z=0.4

Published online by Cambridge University Press:  06 October 2004

David G. Gilbank ,
F. J. Castander ,
M. L. Balogh  and
R. G. Bower
David G. Gilbank
Affiliation:
Department of Astronomy and Astrophysics, University of Toronto, 60 St George Street, Toronto, Ontario, Canada, M5S 3HE email: [email protected]
F. J. Castander
Affiliation:
Institut d'Estudis Espacials de Catalunya/CSIC Gran Capità 2-4, 08034, Barcelona, Spain
M. L. Balogh
Affiliation:
Institute for Computational Cosmology, University of Durham, South Road, Durham, DH1 3LE, UK
R. G. Bower
Affiliation:
Institute for Computational Cosmology, University of Durham, South Road, Durham, DH1 3LE, UK
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present preliminary results from a wide-field spectroscopic survey of two galaxy clusters at $z=0.4$, separated by $\lt$10 $h^{-1}$ Mpc on the sky. Both clusters are similarly optically rich, have velocity dispersions $\sim 700$ km s$^{-1}$, but differ in X-ray luminosity by a factor of $\sim$20.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. 95 - 97
Copyright
© 2004 International Astronomical Union