Using the magnetic dipole method, magnetic field models of eight stars were built in order to obtain additional information about the features of the magnetic field structures in CP stars. These data are necessary to clarify the conditions of star formation in the early stages of stellar evolution. We noticed a large variety of initial conditions that lead to a strong scatter of parameters of magnetic stars and magnetic structures.
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Yu. V. Glagolevskij (2014) studied this question.
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