Cite
HARVARD Citation
Loi, S. (2021). Topology and obliquity of core magnetic fields in shaping seismic properties of slowly rotating evolved stars. Monthly notices of the Royal Astronomical Society. 504 (3), pp. 3711-3729. [Online].
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Loi, S. (2021). Topology and obliquity of core magnetic fields in shaping seismic properties of slowly rotating evolved stars. Monthly notices of the Royal Astronomical Society. 504 (3), pp. 3711-3729. [Online].