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 &; Astrophysics 704 (2025).

Is a 1D perturbative method sufficient for asteroseismic modelling of ;2 Cephei pulsators?
J. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D. Reese, J. Ballot, (2025).

Interior rotation modelling of the ;2 Cep pulsator HD 192575 including multiplet asymmetries
V. Vanlaer, D.M. Bowman, S. Burssens, S.B. Das, L.A. Bugnet, S. Mathis, C. Aerts, Astronomy &; Astrophysics 701 (2025).

Supergranular-scale solar convection not explained by mixing-length theory
C.S. Hanson, S.B. Das, P. Mani, S. Hanasoge, K.R. Sreenivasan, Nature Astronomy 8 (2024) 1088–1101.

Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars
S. Bhattacharya, S.B. Das, L.A. Bugnet, S. Panda, S.M. Hanasoge, Astrophysical Journal 970 (2024).

Unveiling complex magnetic field configurations in red giant stars
S.B. Das, L. Einramhof, L.A. Bugnet, Astronomy &; Astrophysics 690 (2024).