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• W3106599438 startingPage "123" @default.
• W3106599438 abstract "Abstract Rotation has two main qualitative effects on the structure of a star: it distorts the shape and it reduces the total luminosity. The luminosity depends only on the total angular momentum but the shape, and so the observable properties, depends on the internal distribution of angular momentum. The expected distribution, even for main-sequence stars, is an unsolved problem. Redistribution of angular momentum can occur as a result of large-scale circulation currents, instabilities and magnetic stresses and there may be no steady state. If shear instabilities are dominant, then stars may rotate nearly uniformly. Studies of non-radial oscillations might perhaps eventually lead to a direct probing of the internal angular momentum distribution by the methods now being used to study the internal rotation of the Sun. Differential rotation near the surface would probably give rise to turbulent motions, which could generate the mechanical energy flux which seems to be a necessary input to the winds in hot stars." @default.
• W3106599438 created "2020-12-07" @default.
• W3106599438 creator A5089870540 @default.
• W3106599438 date "1987-08-01" @default.
• W3106599438 modified "2023-10-18" @default.
• W3106599438 title "Rotating Stellar Interiors (Review Paper)" @default.
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• W3106599438 doi "https://doi.org/10.1017/s0252921100116148" @default.
• W3106599438 hasPublicationYear "1987" @default.
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