THE POPULATION OF GALAXIES IN THE DISTANT CLUSTERS CL1613+3104 AND CL1600+4109

We study the photometric properties and content of the distant cluster s of galaxies Cl 1613+3104 (z = 0.415) and Cl 1600+4109 (z = 0.540). T he former is a rich, concentrated cluster which shows a strong evidenc e for segregation in luminosity and color. Its population of galaxies separates into two different kinds of objects: a red population compat ible with the colors expected for E/S0 galaxies located preferentially in the central part of the cluster, and a sparse blue population expl ained in part by the presence of normal S/Im galaxies, which is much l ess concentrated. In the case of Cl 1600+4109, there is a lack of E/S0 galaxies and the population is mainly made up of S/Im galaxies, witho ut any evidence of segregation in magnitude or in color. Both clusters exhibit an important fraction of blue objects, increasing with magnit ude. This result is due in part to the presence of normal S/Im galaxie s, and also to extremely blue objects probably undergoing an episode o f intense star-formation.