A High Fraction of Mergers in the cluster MS 1054 – 03 at

We used the Hubble Space Telescope to take a wide field, multicolor image of the high redshift cluster MS1054–03 at z = 0.83. The Keck telescope was used to take 200 redshifts in the field. We have a total of 81 spectroscopically confirmed cluster members with deep WFPC2 imaging. A surprisingly large number of these cluster members are mergers: 13 out of 77 galaxies are classified as merger remnants, or mergers in progress. Most of these are red, and massive. Their restframe B luminosities are amongst the brightest in the cluster: we find that 5 out of the brightest 16 are mergers. No such bright mergers were found in a lower redshift cluster with similar wide field coverage. The mergers in MS1054–03 are preferentially found in the outskirts of the cluster. The distribution of pairs in the outskirts of the cluster shows an excess of galaxies with separation < 10 hkpc, which is independent confirmation of the enhanced interaction rate. The fraction of mergers (17 %) is comparable to the fraction of ellipticals (22 %). Hence up to 50 % of low redshift ellipticals may have formed through mergers since z = 1. There is no evidence for strong star formation in most of the mergers. The mean stellar ages of the mergers may therefore be much older than the “assembly age”, i.e., the age since the time the system was put together. These new results are qualitatively consistent with predictions from hierarchical galaxy formation, and are inconsistent with an early collapse for all early type galaxies.