{"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","department":[{"_id":"LiBu"}],"type":"research_data_reference","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png"},"status":"public","ddc":["520"],"license":"https://creativecommons.org/licenses/by/4.0/","date_updated":"2026-07-22T06:20:53Z","date_created":"2026-01-05T08:39:33Z","date_published":"2025-11-11T00:00:00Z","day":"11","doi":"10.5281/ZENODO.17580178","author":[{"full_name":"Mombarg, Joey","first_name":"Joey","last_name":"Mombarg"},{"full_name":"Vanlaer, Vincent","first_name":"Vincent","last_name":"Vanlaer"},{"first_name":"Srijan B","full_name":"Das, Srijan B","id":"9ce7c423-dacf-11ed-8942-e09c6cb27149","orcid":"0000-0003-0896-7972","last_name":"Das"},{"last_name":"Rieutord","full_name":"Rieutord, Michel","first_name":"Michel"},{"last_name":"Aerts","full_name":"Aerts, Conny","first_name":"Conny"},{"full_name":"Bugnet, Lisa Annabelle","first_name":"Lisa Annabelle","orcid":"0000-0003-0142-4000","id":"d9edb345-f866-11ec-9b37-d119b5234501","last_name":"Bugnet"},{"full_name":"Mathis, Stephane","first_name":"Stephane","last_name":"Mathis"},{"first_name":"Daniel","full_name":"Reese, Daniel","last_name":"Reese"},{"last_name":"Ballot","full_name":"Ballot, Jerome","first_name":"Jerome"}],"citation":{"apa":"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>","ieee":"J. Mombarg <i>et al.</i>, “Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?” Zenodo, 2025.","ista":"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>.","mla":"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>.","chicago":"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>.","ama":"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>","short":"J. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D. Reese, J. Ballot, (2025)."},"abstract":[{"text":"Supplementary material for Mombarg et al. (2025, A&A). Title: \"Is a 1D perturbative method sufficient for asteroseismic modelling of \r\n~Cephei pulsators? Implications for measurements of rotation and internal magnetic fields\"\r\n\r\nContent:\r\n- 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.\r\n\r\n- 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)\r\n\r\n- 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)","lang":"eng"}],"publisher":"Zenodo","article_processing_charge":"No","main_file_link":[{"url":"https://doi.org/10.5281/zenodo.17580178","open_access":"1"}],"OA_type":"gold","year":"2025","OA_place":"repository","title":"Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?","month":"11","oa_version":"Published Version","oa":1,"_id":"20936","related_material":{"record":[{"relation":"used_in_publication","status":"public","id":"20931"}]}}