thesis Joey Mombarg author Vincent Vanlaer author Srijan B Das author 9ce7c423-dacf-11ed-8942-e09c6cb271490000-0003-0896-7972 Michel Rieutord author Conny Aerts author Lisa Annabelle Bugnet author d9edb345-f866-11ec-9b37-d119b52345010000-0003-0142-4000 Stephane Mathis author Daniel Reese author Jerome Ballot author LiBu department Supplementary material for Mombarg et al. (2025, A&A). Title: "Is a 1D perturbative method sufficient for asteroseismic modelling of ~Cephei pulsators? Implications for measurements of rotation and internal magnetic fields" Content: - Non-rotating ESTER models and associated .GSM models. (Xini = 0.71, Zini = 0.014, vertical/horizonal viscosity 10^7 cm^2/s, vertical chemical diffusion 10^4 cm^2/s for evolution model. More details on the ESTER models can be found in the ESTER manual. - Rotational asymmetries computed with StORM and TOP in 1/d, and the central m=0 frequency from TOP in 1/d. (all_A*_new.pkl) - Magnetic asymmetries in 1/d for different obliquity angles between 0 and 90 deg for ZAMS and MAMS model, for B_0 = 75 kG. *_nu key gives unperturbed mode frequencies, *_npg the radial order (asym_dict.pkl, asym_dict_evol.pkl) Zenodo2025 10.5281/ZENODO.17580178 https://research-explorer.ista.ac.at/record/20931 J. Mombarg <i>et al.</i>, “Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?” Zenodo, 2025. Mombarg J, Vanlaer V, Das SB, et al. Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators? 2025. doi:<a href="https://doi.org/10.5281/ZENODO.17580178">10.5281/ZENODO.17580178</a> Mombarg, J., Vanlaer, V., Das, S. B., Rieutord, M., Aerts, C., Bugnet, L. A., … Ballot, J. (2025). Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators? Zenodo. <a href="https://doi.org/10.5281/ZENODO.17580178">https://doi.org/10.5281/ZENODO.17580178</a> Mombarg, Joey, Vincent Vanlaer, Srijan B Das, Michel Rieutord, Conny Aerts, Lisa Annabelle Bugnet, Stephane Mathis, Daniel Reese, and Jerome Ballot. “Is a 1D Perturbative Method Sufficient for Asteroseismic Modelling of β Cephei Pulsators?” Zenodo, 2025. <a href="https://doi.org/10.5281/ZENODO.17580178">https://doi.org/10.5281/ZENODO.17580178</a>. Mombarg, Joey, et al. <i>Is a 1D Perturbative Method Sufficient for Asteroseismic Modelling of β Cephei Pulsators?</i> Zenodo, 2025, doi:<a href="https://doi.org/10.5281/ZENODO.17580178">10.5281/ZENODO.17580178</a>. Mombarg J, Vanlaer V, Das SB, Rieutord M, Aerts C, Bugnet LA, Mathis S, Reese D, Ballot J. 2025. Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?, Zenodo, <a href="https://doi.org/10.5281/ZENODO.17580178">10.5281/ZENODO.17580178</a>. J. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D. Reese, J. Ballot, (2025). 209362026-01-05T08:39:33Z2026-07-22T06:20:53Z