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Cited article:

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Monthly Notices of the Royal Astronomical Society 520 (4) 5573 (2023)
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The first two-dimensional stellar structure and evolution models of rotating stars

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Evolution of rotation in rapidly rotating early-type stars during the main sequence with 2D models

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An algorithm for computing the 2D structure of fast rotating stars: Part I steady solutions

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https://doi.org/10.1016/j.jcp.2016.05.011

Pulsation modes in rapidly rotating stellar models based on the self-consistent field method

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Diagnoses to unravel secular hydrodynamical processes in rotating main sequence stars

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Joint Discussion 17 Highlights of recent progress in the seismology of the Sun and Sun-like stars

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