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This paper considers a system modelling the evolution of a rigid body immersed in a bidimensional incompressible perfect fluid. In the special case of a disk-shaped rigid body, it was shown by C. Rosier and L. Rosier (2009) that the system admits a unique global solution when the initial fluid velocity belongs to () and its vorticity lies in with . By establishing a Beale-Kato-Majda type bound, we generalize the result by removing the constraint and allowing the rigid body to be of arbitrary shape. Moreover, we obtain an explicit energy bound.

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