In this review (part I) the most important results of research on the properties of the magnetic fields of chemically peculiar stars prior to 2000 are examined critically. The properties of the magnetic fields are examined from the standpoint of their conformity with the relict hypothesis. Later results will be discussed in part II.
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Translated from Astrofizika, Vol. 61, No. 3, pp. 459-484 (August 2018).
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Glagolevskij, Y.V. Progress in Studies of the Evolution of the Magnetic Fields of CP-Stars. I. Astrophysics 61, 413–434 (2018). https://doi.org/10.1007/s10511-018-9547-4
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DOI: https://doi.org/10.1007/s10511-018-9547-4