We investigated the galaxy morphology of 6 Abell clusters at z = 0:0784 - 0:145 based on deep images obtained using MegaCam on the CFHT. For hundreds of galaxies in our data, we classified their mor- phology based on criteria related to secular or merger related evolution. We found that the morphological mixture of galaxies varies considerably from cluster to cluster. This article contains a general description of our deep imaging campaign and preliminary results for galaxy morphologies in cluster environments.

ABSTRACT
1. INTRODUCTION
2. THE DEEP IMAGING SURVEY OF GALAXY CLUS-TERS
3. SAMPLE AND VISUAL CLASSIFICATION
4. SUMMARY
REFERENCES

• Seulhee Oh(Department of Astronomy, Yonsei University)
• Sukyoung K. Yi(Department of Astronomy, Yonsei University)