A possible scenario is proposed for the origin and evolution of magnetic stars based on the observational data accumulated up to now. The large difference in magnetic structures and the predominant orientation of the magnetic dipoles are explained, along with the mechanism by which 10% of the magnetic stars differ from normal. A reason is discovered for the slow axial rotation of the stars and a cause is found for the absence of strong magnetic fields in Ae/Be Herbig stars.
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Translated from Astrofizika, Vol. 57, No. 3, pp. 337-354 (August 2014).
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Glagolevskij, Y.V. Evolution of the Magnetic Fields of Main-Sequence CP-Stars. IV. Astrophysics 57, 315–329 (2014). https://doi.org/10.1007/s10511-014-9337-6
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DOI: https://doi.org/10.1007/s10511-014-9337-6