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What has prevented the formation of a strong bar in the majority of disc galaxies? No truly satisfactory answer has yet been given to this question and the difficulty remains a major obstacle to our understanding of the dynamics of these systems. In this review, I will discuss the implications of recent studies of this problem.doi:10.1017/s0074180900032812 fatcat:dy6u6oyfbbfe3dsyxc6fdrt3bm