Features of magnetic field structures in chemically peculiar stars. IV


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We present results of modeling of the sample of magnetic stars. We have obtained such important for magnetic star physics parameters as the mean surface magnetic field Bs, the magnetic field at magnetic poles—Bp, the dipole inclination to the rotation equatorial plane α, and the distance to monopoles from the center of the star Δa. We present some information onmagnetic star physics that helps to understand the derived results better.

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Yu. Glagolevskij

Special Astrophysical Observatory

编辑信件的主要联系方式.
Email: glagol@sao.ru
俄罗斯联邦, Nizhnii Arkhyz, 369167

A. Nazarenko

Special Astrophysical Observatory

Email: glagol@sao.ru
俄罗斯联邦, Nizhnii Arkhyz, 369167

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