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We study the evolution of circumstellar massive disks around the primary starof a binary system focusing on the computation of disk eccentricity. Inparticular, we concentrate on its dependence on the binary eccentricity.Self-gravity is included in our numerical simulations. Our standard modelassumes a semimajor axis for the binary of 30 AU, the most probable valueaccording to the present binary statistics.

On the eccentricity of self-gravitating circumstellar disks in eccentric binary systems