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Secular Stability of Magnetic Field Structures in Magnetic CP-Stars

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Astrophysics Aims and scope

The magnetic field structures of stars with different ages are studied. No changes in the position and orientation of magnetic dipoles with age are observed. It is concluded that there are no global motions, such as differential rotation meridional circulation, etc., inside magnetic stars. Arguments are presented in favor of the assumption that magnetic stars rotate as solids. These conclusions do not concern the behavior of convective cores.

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Authors and Affiliations

  1. Special Astrophysical Observatory, Russian Academy of Sciences, Moscow, Russia

    Yu. V. Glagolevskij & A. F. Nazarenko

Authors
  1. Yu. V. Glagolevskij
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  2. A. F. Nazarenko
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Correspondence to Yu. V. Glagolevskij.

Additional information

Translated from Astrofizika, Vol. 62, No. 4, pp. 547-558 (November 2019)

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Glagolevskij, Y.V., Nazarenko, A.F. Secular Stability of Magnetic Field Structures in Magnetic CP-Stars. Astrophysics 62, 491–501 (2019). https://doi.org/10.1007/s10511-019-09598-z

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  • DOI: https://doi.org/10.1007/s10511-019-09598-z

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