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Generalized Rotation

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The Roche Problem

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 152))

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Abstract

In the preceding five chapters of this book we have been concerned with the effects produced by uni-axial rotation on the shape of self-gravitating fluids of arbitrary structure. There was a good reason for that; for all stars observed so far in the sky, whether single or components of multiple systems, are found to be endowed with rotation—no doubt as a consequence of the vorticity in pre-existing gas (or plasma), from which the stars originate by contraction. The angular momentum associated with rotation—conserved over long evolutionary epochs—represents as fundamental a property with which stars embark on their celestial careers as their initial masses and chemical composition.

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© 1989 Kluwer Academic Publishers

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Kopal, Z. (1989). Generalized Rotation. In: The Roche Problem. Astrophysics and Space Science Library, vol 152. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2291-4_6

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  • DOI: https://doi.org/10.1007/978-94-009-2291-4_6

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7528-2

  • Online ISBN: 978-94-009-2291-4

  • eBook Packages: Springer Book Archive

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