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Structure-distortion of polytropic stars by differential rotation: Third-order perturbation theory

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Abstract

In order to specify the structure of a rapidly and differentially rotating gaseous polytrope, we extend Chandrasekhar's perturbation theory to include third-order terms in the perturbation parameter. In the present paper, the theory developed is required for a subsequent numerical treatment of the structure-determination.

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References

  • Chandrasekhar, S.: 1939,Stellar Structure, Dover Publications.

  • Chandrasekhar, S. and Lebovitz, N.: 1962,Astrophys J. 137, 1082.

    Google Scholar 

  • Clement, M. J.: 1967,Astrophys. J. 150, 589.

    Google Scholar 

  • Geroyannis, V. S., Tokis, J. N. and Valvi, F. M.: 1979,Astrophys Space Sci. 64, 359.

    Google Scholar 

  • Kovetz, A.: 1968,Astrophys. J. 154 999.

    Google Scholar 

  • Stoeckly, R.: 1965,Astrophys. J. 142, 208.

    Google Scholar 

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This research was supported by the Research Development Project of the University of Patras, Greece.

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Geroyannis, V.S., Antonakopoulos, G.A. Structure-distortion of polytropic stars by differential rotation: Third-order perturbation theory. Astrophys Space Sci 74, 97–110 (1981). https://doi.org/10.1007/BF00642085

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  • DOI: https://doi.org/10.1007/BF00642085

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