Is a 1D perturbative method sufficient for asteroseismic modelling of ;2 Cephei pulsators? Implications for measurements of rotation and internal magnetic fields
J.S.G. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D.R. Reese, J. Ballot, Astronomy and Astrophysics 704 (2025).