The behavior of magnetic stars near the Zero Age Main Sequence (ZAMS) is considered. The paper shows that the most probable reason for the negative results of the search for magnetic fields in HAeBe stars is turbulence caused by the burning of deuterium. The magnetic field variability and other properties of stars are studied as they move along the evolutionary path.
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Yu. V. Glagolevskij (2021) studied this question.
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