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Early-type dwarf galaxies are found to have high specific globular clusterfrequencies which are similar to the high S values that are observed inluminous galaxies of types E and S0. It appears unlikely that cluster formationduring mergers between dwarf disk systems can account for the high specificglobular cluster frequency that is observed in early-type dwarf galaxies. Somealternative scenarios are briefly discussed.

Some Constraints on Galaxy Evolution Imposed by the Specific Frequency of Globular Clusters