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 and 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 and 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: 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
 
[2]
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
 
[1]
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
 
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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 and 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 and 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: 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
 
[2]
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
 
[1]
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
 
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  • 5 OA Fulltext(s)

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