6 Publications

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[6]
2025 | Published | Journal Article | IST-REx-ID: 20350 | OA | PlanS
Vanlaer, V., Bowman, D. M., Burssens, S., Das, S. B., Bugnet, L. A., Mathis, S., & Aerts, C. (2025). Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202452885
[Published Version] View | Files available | DOI | WoS | arXiv
 
[5]
2025 | Published | Journal Article | IST-REx-ID: 20931 | OA | PlanS
Mombarg, J. S. G., 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? Implications for measurements of rotation and internal magnetic fields. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202557247
[Published Version] View | Files available | DOI | arXiv
 
[4]
2025 | Research Data Reference | IST-REx-ID: 20936 | OA
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. https://doi.org/10.5281/ZENODO.17580178
[Submitted Version] View | Files available | DOI | Download Submitted Version (ext.)
 
[3]
2024 | Published | Journal Article | IST-REx-ID: 17189
Hanson, C. S., Das, S. B., Mani, P., Hanasoge, S., & Sreenivasan, K. R. (2024). Supergranular-scale solar convection not explained by mixing-length theory. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-024-02304-w
View | DOI | WoS
 
[2]
2024 | Published | Journal Article | IST-REx-ID: 17326 | OA
Bhattacharya, S., Das, S. B., Bugnet, L. A., Panda, S., & Hanasoge, S. M. (2024). Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars. Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ad4708
[Published Version] View | Files available | DOI | WoS | arXiv
 
[1]
2024 | Published | Journal Article | IST-REx-ID: 18528 | OA
Das, S. B., Einramhof, L., & Bugnet, L. A. (2024). Unveiling complex magnetic field configurations in red giant stars. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202450918
[Published Version] View | Files available | DOI | WoS | arXiv
 

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6 Publications

Mark all

[6]
2025 | Published | Journal Article | IST-REx-ID: 20350 | OA | PlanS
Vanlaer, V., Bowman, D. M., Burssens, S., Das, S. B., Bugnet, L. A., Mathis, S., & Aerts, C. (2025). Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202452885
[Published Version] View | Files available | DOI | WoS | arXiv
 
[5]
2025 | Published | Journal Article | IST-REx-ID: 20931 | OA | PlanS
Mombarg, J. S. G., 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? Implications for measurements of rotation and internal magnetic fields. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202557247
[Published Version] View | Files available | DOI | arXiv
 
[4]
2025 | Research Data Reference | IST-REx-ID: 20936 | OA
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. https://doi.org/10.5281/ZENODO.17580178
[Submitted Version] View | Files available | DOI | Download Submitted Version (ext.)
 
[3]
2024 | Published | Journal Article | IST-REx-ID: 17189
Hanson, C. S., Das, S. B., Mani, P., Hanasoge, S., & Sreenivasan, K. R. (2024). Supergranular-scale solar convection not explained by mixing-length theory. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-024-02304-w
View | DOI | WoS
 
[2]
2024 | Published | Journal Article | IST-REx-ID: 17326 | OA
Bhattacharya, S., Das, S. B., Bugnet, L. A., Panda, S., & Hanasoge, S. M. (2024). Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars. Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ad4708
[Published Version] View | Files available | DOI | WoS | arXiv
 
[1]
2024 | Published | Journal Article | IST-REx-ID: 18528 | OA
Das, S. B., Einramhof, L., & Bugnet, L. A. (2024). Unveiling complex magnetic field configurations in red giant stars. Astronomy and Astrophysics. EDP Sciences. https://doi.org/10.1051/0004-6361/202450918
[Published Version] View | Files available | DOI | WoS | arXiv
 

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