December 1, 1967

Slowly Rotating Relativistic Stars. I. Equations of Structure

JHJames B. HartleUniversity of California, Santa Barbara

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Resumen

Equations are given for the calculation of the equilibrium configurations of slowly rotating stars in the framework of general relativity. The rotation is treated to second order in the angular velocity, but no other approximation is made.

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James B. Hartle (Fri,) studied this question.

synapsesocial.com/papers/6a00ebca6018b8d0892dda6e https://doi.org/https://doi.org/10.1086/149400

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