DOI,IST REx ID,Research Group,Title of publication
10.1051/0004-6361/202557247,20931,LiBu,Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators? Implications for measurements of rotation and internal magnetic fields
10.5281/ZENODO.17580178,20936,LiBu,Is a 1D perturbative method sufficient for asteroseismic modelling of β Cephei pulsators?
10.1051/0004-6361/202452885,20350,LiBu,Interior rotation modelling of the β Cep pulsator HD 192575 including multiplet asymmetries
10.1038/s41550-024-02304-w,17189,LiBu,Supergranular-scale solar convection not explained by mixing-length theory
10.3847/1538-4357/ad4708,17326,LiBu,Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main-sequence stars
10.1051/0004-6361/202450918,18528,LiBu,Unveiling complex magnetic field configurations in red giant stars