Srijan B Das
6 Publications
2025 |
Published |
Journal Article |
IST-REx-ID: 20350 |
| 
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Vanlaer, V., et al. “Interior Rotation Modelling of the β Cep Pulsator HD 192575 Including Multiplet Asymmetries.” Astronomy & Astrophysics, vol. 701, A5, EDP Sciences, 2025, doi:10.1051/0004-6361/202452885.
[Published Version]
View
| Files available
| DOI
| WoS
| arXiv
2025 |
Published |
Journal Article |
IST-REx-ID: 20931 |
|
|
Mombarg, J. S. G., et al. “Is a 1D Perturbative Method Sufficient for Asteroseismic Modelling of β Cephei Pulsators? Implications for Measurements of Rotation and Internal Magnetic Fields.” Astronomy & Astrophysics, vol. 704, A336, EDP Sciences, 2025, doi:10.1051/0004-6361/202557247.
[Published Version]
View
| Files available
| DOI
| arXiv
2025 |
Research Data Reference |
IST-REx-ID: 20936 |
Mombarg, Joey, et al. Is a 1D Perturbative Method Sufficient for Asteroseismic Modelling of β Cephei Pulsators? Zenodo, 2025, doi:10.5281/ZENODO.17580178.
[Submitted Version]
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| Files available
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| Download Submitted Version (ext.)
2024 |
Published |
Journal Article |
IST-REx-ID: 18528 |
Das, Srijan B., et al. “Unveiling Complex Magnetic Field Configurations in Red Giant Stars.” Astronomy and Astrophysics, vol. 690, A217, EDP Sciences, 2024, doi:10.1051/0004-6361/202450918.
[Published Version]
View
| Files available
| DOI
| WoS
| arXiv
2024 |
Published |
Journal Article |
IST-REx-ID: 17189
Hanson, Chris S., et al. “Supergranular-Scale Solar Convection Not Explained by Mixing-Length Theory.” Nature Astronomy, vol. 8, Springer Nature, 2024, pp. 1088–101, doi:10.1038/s41550-024-02304-w.
View
| DOI
| WoS
2024 |
Published |
Journal Article |
IST-REx-ID: 17326 |
Bhattacharya, Shatanik, et al. “Detectability of Axisymmetric Magnetic Fields from the Core to the Surface of Oscillating Post-Main-Sequence Stars.” Astrophysical Journal, vol. 970, no. 1, 42, IOP Publishing, 2024, doi:10.3847/1538-4357/ad4708.
[Published Version]
View
| Files available
| DOI
| WoS
| arXiv
Grants
6 Publications
2025 |
Published |
Journal Article |
IST-REx-ID: 20350 |
|
|
Vanlaer, V., et al. “Interior Rotation Modelling of the β Cep Pulsator HD 192575 Including Multiplet Asymmetries.” Astronomy & Astrophysics, vol. 701, A5, EDP Sciences, 2025, doi:10.1051/0004-6361/202452885.
[Published Version]
View
| Files available
| DOI
| WoS
| arXiv
2025 |
Published |
Journal Article |
IST-REx-ID: 20931 |
|
|
Mombarg, J. S. G., et al. “Is a 1D Perturbative Method Sufficient for Asteroseismic Modelling of β Cephei Pulsators? Implications for Measurements of Rotation and Internal Magnetic Fields.” Astronomy & Astrophysics, vol. 704, A336, EDP Sciences, 2025, doi:10.1051/0004-6361/202557247.
[Published Version]
View
| Files available
| DOI
| arXiv
2025 |
Research Data Reference |
IST-REx-ID: 20936 |
Mombarg, Joey, et al. Is a 1D Perturbative Method Sufficient for Asteroseismic Modelling of β Cephei Pulsators? Zenodo, 2025, doi:10.5281/ZENODO.17580178.
[Submitted Version]
View
| Files available
| DOI
| Download Submitted Version (ext.)
2024 |
Published |
Journal Article |
IST-REx-ID: 18528 |
Das, Srijan B., et al. “Unveiling Complex Magnetic Field Configurations in Red Giant Stars.” Astronomy and Astrophysics, vol. 690, A217, EDP Sciences, 2024, doi:10.1051/0004-6361/202450918.
[Published Version]
View
| Files available
| DOI
| WoS
| arXiv
2024 |
Published |
Journal Article |
IST-REx-ID: 17189
Hanson, Chris S., et al. “Supergranular-Scale Solar Convection Not Explained by Mixing-Length Theory.” Nature Astronomy, vol. 8, Springer Nature, 2024, pp. 1088–101, doi:10.1038/s41550-024-02304-w.
View
| DOI
| WoS
2024 |
Published |
Journal Article |
IST-REx-ID: 17326 |
Bhattacharya, Shatanik, et al. “Detectability of Axisymmetric Magnetic Fields from the Core to the Surface of Oscillating Post-Main-Sequence Stars.” Astrophysical Journal, vol. 970, no. 1, 42, IOP Publishing, 2024, doi:10.3847/1538-4357/ad4708.
[Published Version]
View
| Files available
| DOI
| WoS
| arXiv