
doi: 10.1063/1.2818985
The treatment of rotating stars brings together several stellar astrophysical disciplines. Models of rotating stars must be able to simulate the stellar structure and evolution, stellar atmospheres models are required to determine the spectral energy distribution and spectral line shapes of rotating stars, and radial and nonradial stellar pulsation is needed to determine the modes in which such stars might pulsate. Here we discuss bringing together all the needed information to construct a rotating stars toolkit.
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