An approximate global stationary axisymmetric solution of the Einstein equations

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In this work we present an approximate solution of the Einstein equations describing a global model for the gravitational field generated by a bounded, self-gravitating stationary and axisymmetric body rotating rigidly with constant angular velocity.
12 pages, LaTeX, conference done at Spanish Relativity Meeting (Alicante, Spain, 2003). A few minor errata have been corrected. A formula for pressure is also added

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