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Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?
J. S. G. Mombarg, V. Vanlaer, S. B. Das, M. Rieutord, C. Aerts, L. Bugnet, S. Mathis, D. R. Reese and J. Ballot Astronomy & Astrophysics 704 A336 (2025) https://doi.org/10.1051/0004-6361/202557247
Approaching the structure of rotating bodies from dimension reduction