Rotational distortion of stars having ar
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M. Bahgat El-Shaarawy
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Article
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1989
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Springer Netherlands
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English
β 498 KB
In a series of papers, the equilibrium configurations of highly rotating fluid bodies have been derived. The deformation of these inhomogeneous self-gravitating fluid, of arbitrary internal structure are due to centrifugation potential. These level surfaces are expressed in terms of fourth-order sec