Srijan B Das

6 Publications

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[6]
2025 | Published | Journal Article | IST-REx-ID: 20350 | OA | PlanS
Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries
V. Vanlaer, D.M. Bowman, S. Burssens, S.B. Das, L.A. Bugnet, S. Mathis, C. Aerts, Astronomy & Astrophysics 701 (2025).
[Published Version] View | Files available | DOI | WoS | arXiv
 
[5]
2025 | Published | Journal Article | IST-REx-ID: 20931 | OA | PlanS
Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators? Implications for measurements of rotation and internal magnetic fields
J.S.G. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D.R. Reese, J. Ballot, Astronomy & Astrophysics 704 (2025).
[Published Version] View | Files available | DOI | arXiv
 
[4]
2025 | Research Data Reference | IST-REx-ID: 20936 | OA
Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?
J. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D. Reese, J. Ballot, (2025).
[Submitted Version] View | Files available | DOI | Download Submitted Version (ext.)
 
[3]
2024 | Published | Journal Article | IST-REx-ID: 18528 | OA
Unveiling complex magnetic field configurations in red giant stars
S.B. Das, L. Einramhof, L.A. Bugnet, Astronomy and Astrophysics 690 (2024).
[Published Version] View | Files available | DOI | WoS | arXiv
 
[2]
2024 | Published | Journal Article | IST-REx-ID: 17189
Supergranular-scale solar convection not explained by mixing-length theory
C.S. Hanson, S.B. Das, P. Mani, S. Hanasoge, K.R. Sreenivasan, Nature Astronomy 8 (2024) 1088–1101.
View | DOI | WoS
 
[1]
2024 | Published | Journal Article | IST-REx-ID: 17326 | OA
Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars
S. Bhattacharya, S.B. Das, L.A. Bugnet, S. Panda, S.M. Hanasoge, Astrophysical Journal 970 (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
Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries
V. Vanlaer, D.M. Bowman, S. Burssens, S.B. Das, L.A. Bugnet, S. Mathis, C. Aerts, Astronomy & Astrophysics 701 (2025).
[Published Version] View | Files available | DOI | WoS | arXiv
 
[5]
2025 | Published | Journal Article | IST-REx-ID: 20931 | OA | PlanS
Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators? Implications for measurements of rotation and internal magnetic fields
J.S.G. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D.R. Reese, J. Ballot, Astronomy & Astrophysics 704 (2025).
[Published Version] View | Files available | DOI | arXiv
 
[4]
2025 | Research Data Reference | IST-REx-ID: 20936 | OA
Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?
J. Mombarg, V. Vanlaer, S.B. Das, M. Rieutord, C. Aerts, L.A. Bugnet, S. Mathis, D. Reese, J. Ballot, (2025).
[Submitted Version] View | Files available | DOI | Download Submitted Version (ext.)
 
[3]
2024 | Published | Journal Article | IST-REx-ID: 18528 | OA
Unveiling complex magnetic field configurations in red giant stars
S.B. Das, L. Einramhof, L.A. Bugnet, Astronomy and Astrophysics 690 (2024).
[Published Version] View | Files available | DOI | WoS | arXiv
 
[2]
2024 | Published | Journal Article | IST-REx-ID: 17189
Supergranular-scale solar convection not explained by mixing-length theory
C.S. Hanson, S.B. Das, P. Mani, S. Hanasoge, K.R. Sreenivasan, Nature Astronomy 8 (2024) 1088–1101.
View | DOI | WoS
 
[1]
2024 | Published | Journal Article | IST-REx-ID: 17326 | OA
Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars
S. Bhattacharya, S.B. Das, L.A. Bugnet, S. Panda, S.M. Hanasoge, Astrophysical Journal 970 (2024).
[Published Version] View | Files available | DOI | WoS | arXiv
 
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