The dynamical status of the cluster of galaxies 1E0657-56^*

¹ Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
² INAF, Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, 34131 Trieste, Italy
³ Smithsonian Institution, F. L. Whipple Observatory, PO Box 97, 670 Mount Hopkins, Amado, AZ 85645, USA
⁴ Universitäts-Sternwarte, Scheinerstrasse 1, 81679 Muenchen, Germany

Corresponding author: A. Biviano, biviano@ts.astro.it

Received: 19 December 2001
Accepted: 12 February 2002

Abstract

We present the results of a new spectroscopic and photometric survey of the hot X-ray cluster , at . We determine the presence of a low velocity dispersion subcluster, which is offset from the main cluster position by 0.7 Mpc and 600 km s^-1. We determine the virial masses and total luminosities of the cluster and its subcluster, and solve for the two-body dynamical model. With additional constraints from the results of the analysis of the cluster X-ray emission by Markevitch et al. ([CITE]), we find that the subcluster passed through the cluster centre 0.15 Gyr ago. Taken at face value the mass of the subcluster is typical of a loose group. It is however difficult to establish the pre-merger mass of the colliding system. We provide tentative evidence that the subcluster is in fact the remnant core of a moderately massive cluster, stripped by the collision with . The main cluster dynamics does not seem to have suffered from this collision. On the contrary, the cluster X-ray properties seem to have been significantly affected. We also discuss the effect of the subcluster collision in relation to starburst events and the cluster radio halo.