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Varvara Butkovskaya
Sergei Plachinda

Abstract

To date, magnetic fields have been detected in various types of pulsating stars. For several of these stars, the variability of the magnetic field with their radial pulsation period was confirmed. The physical mechanism of the pulsation variability of the magnetic field remains unknown. We discuss the current state of the problem of magnetic field variability over pulsation cycles in radially pulsating stars.

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How to Cite
Butkovskaya V., Plachinda S., 2021. Acta Astrophysica Taurica, vols. 3, no. 1, pp. 1–5. DOI: 10.31059/aat.vol3.iss1.pp1-5
Section
Magnetism and activity of the Sun and stars – 2021 Conference proceedings

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