Abstract
We continue our program of the study of large-scale structures of magnetic fields in chemically peculiar stars. In this paper we analyze eight stars, out of which three stars have the structure of a central dipole, three—the structure of a dipole shifted along the axis, and two—of a dipole shifted across the axis. High-precision measurements (with σ = 50 and 80 G) are available for two stars (HD62140 and HD71866, respectively). The model phase dependences agree with the measurements within the errors. This result shows that the hypothesis about the dipole structure of the magnetic fields of CP stars is well founded.
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Original Russian Text © Yu.V. Glagolevskij, 2012, published in Astrofizicheskii Byulleten, 2012, Vol. 67, No. 3, pp. 278–284.
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Glagolevskij, Y.V. Specificities of magnetic field structures in chemically peculiar stars. Astrophys. Bull. 67, 264–270 (2012). https://doi.org/10.1134/S1990341312030030
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DOI: https://doi.org/10.1134/S1990341312030030