Srijan B Das

6 Publications

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[6]
2025 | Published | Journal Article | IST-REx-ID: 20350 | OA | PlanS
V. Vanlaer et al., “Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries,” Astronomy and Astrophysics, vol. 701. EDP Sciences, 2025.
[Published Version] View | Files available | DOI | WoS | arXiv
 
[5]
2025 | Published | Journal Article | IST-REx-ID: 20931 | OA | PlanS
J. S. G. Mombarg 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 and Astrophysics, vol. 704. EDP Sciences, 2025.
[Published Version] View | Files available | DOI | arXiv
 
[4]
2025 | Research Data Reference | IST-REx-ID: 20936 | OA
J. Mombarg et al., “Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?” Zenodo, 2025.
[Submitted Version] View | Files available | DOI | Download Submitted Version (ext.)
 
[3]
2024 | Published | Journal Article | IST-REx-ID: 17189
C. S. Hanson, S. B. Das, P. Mani, S. Hanasoge, and K. R. Sreenivasan, “Supergranular-scale solar convection not explained by mixing-length theory,” Nature Astronomy, vol. 8. Springer Nature, pp. 1088–1101, 2024.
View | DOI | WoS
 
[2]
2024 | Published | Journal Article | IST-REx-ID: 17326 | OA
S. Bhattacharya, S. B. Das, L. A. Bugnet, S. Panda, and S. M. Hanasoge, “Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars,” Astrophysical Journal, vol. 970, no. 1. IOP Publishing, 2024.
[Published Version] View | Files available | DOI | WoS | arXiv
 
[1]
2024 | Published | Journal Article | IST-REx-ID: 18528 | OA
S. B. Das, L. Einramhof, and L. A. Bugnet, “Unveiling complex magnetic field configurations in red giant stars,” Astronomy and Astrophysics, vol. 690. EDP Sciences, 2024.
[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
V. Vanlaer et al., “Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries,” Astronomy and Astrophysics, vol. 701. EDP Sciences, 2025.
[Published Version] View | Files available | DOI | WoS | arXiv
 
[5]
2025 | Published | Journal Article | IST-REx-ID: 20931 | OA | PlanS
J. S. G. Mombarg 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 and Astrophysics, vol. 704. EDP Sciences, 2025.
[Published Version] View | Files available | DOI | arXiv
 
[4]
2025 | Research Data Reference | IST-REx-ID: 20936 | OA
J. Mombarg et al., “Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?” Zenodo, 2025.
[Submitted Version] View | Files available | DOI | Download Submitted Version (ext.)
 
[3]
2024 | Published | Journal Article | IST-REx-ID: 17189
C. S. Hanson, S. B. Das, P. Mani, S. Hanasoge, and K. R. Sreenivasan, “Supergranular-scale solar convection not explained by mixing-length theory,” Nature Astronomy, vol. 8. Springer Nature, pp. 1088–1101, 2024.
View | DOI | WoS
 
[2]
2024 | Published | Journal Article | IST-REx-ID: 17326 | OA
S. Bhattacharya, S. B. Das, L. A. Bugnet, S. Panda, and S. M. Hanasoge, “Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars,” Astrophysical Journal, vol. 970, no. 1. IOP Publishing, 2024.
[Published Version] View | Files available | DOI | WoS | arXiv
 
[1]
2024 | Published | Journal Article | IST-REx-ID: 18528 | OA
S. B. Das, L. Einramhof, and L. A. Bugnet, “Unveiling complex magnetic field configurations in red giant stars,” Astronomy and Astrophysics, vol. 690. EDP Sciences, 2024.
[Published Version] View | Files available | DOI | WoS | arXiv
 
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Citation Style: IEEE

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