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- W1983643974 abstract "A successive perturbation theory is established for the structure of stars in uniform rotation with a known law of energy generation. The first-order structure is computed for a rotating Cowling model with a law of energy generation |$epsilon ,propto ,rho {T}^{17}$| The results from a first-order model indicate that with the distribution of rotation velocities observed, rotation can produce a spread in luminosity of order half a magnitude in a mass-luminosity diagram, and of order half a magnitude for a given spectral type in a colour-magnitude array, this figure being for the most rapidly rotating Be stars." @default.
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- W1983643974 date "1953-12-01" @default.
- W1983643974 modified "2023-09-26" @default.
- W1983643974 title "The Structure of Rotating Stars. I" @default.
- W1983643974 doi "https://doi.org/10.1093/mnras/113.6.701" @default.
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