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Is a 1D perturbative method sufficient for asteroseismic modelling of <i>β</i> Cephei pulsators?

J S G Mombarg et al.
HAL (France) · Papers · License: Open Access
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magneticfieldrotationstars
Magnetic field -stars, Asteroseismology -stars, Rotation, 0, Interiors -stars, Massive -stars
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Record · ID 322508
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