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VOLUME 51 (1990) | ISSUE 10 | PAGE 493
New exact solution of Einstein's equations for the gravitational field of a stationary axisymmetric mass
An exact, asymptotically planar solution of the vacuum Einstein's equations is derived to describe the external gravitational field of a rotating axisymmetric mass. This solution has a static Schwarzschild limit. It contains the Kerr metric as a special case.