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A Numerical Study of the Fission Hypothesis for Rotating Polytropes
Published online by Cambridge University Press: 12 April 2016
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Analytic stability analyses (Lyttleton, 1953; Chandresekhar, 1969) have shown that Maclaurin spheroids are dynamically unstable to non-axisymmetric perturbations if
- Type
- I. ID, 2D, and 3D Collapse of Interstellar Clouds
- Information
- International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 267 - 273
- Copyright
- Copyright © Reidel 1980
References
Chandrasekhar, S.: 1969, Ellipsoidal Figures of Equilibrium, Yale Univ. Press, New Haven.Google Scholar
Gingold, R. A., and Monaghan, J. J.: 1978, Monthly Notices Roy. Astron. Soc. 184, p. 481.CrossRefGoogle Scholar
Gingold, R. A., and Monaghan, J. J.: 1979, Monthly Notices Roy. Astron. Soc. 188, p. 39.Google Scholar
Jeans, J. H.: 1919, Problems of Cosmology and Stellar Dynamics, Cambridge Univ. Press, Cambridge.Google Scholar
Lyttleton, R. A.: 1953, The Stability of Rotating Liquid Masses, Cambridge Univ. Press, Cambridge.Google Scholar