CAOSP abstracts, Volume: 48, No.: 1, year: 2018

Abstract: Precision asteroseismology requires a detailed modelling of stellar structure and pulsations. It means that even if some effects are small they must be taken into account for an accurate confrontation of theory and observations. Studies of the last decade have shown that magnetic field is quite ubiquitous among stellar objects. Thus, by studying pulsators with measurable magnetic filed one can derive seismic inferences about a distortion caused by the magnetic field inaccessible in other manner. Here we discuss the latest achievements of synergies between asteroseismic inferences and magnetic field measurements.