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
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