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Structure of the Magnetic Field of the Star HD133880 (Si)

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The magnetic field of the star HD133880 is modeled assuming a magnetic field structure that is described by two theoretical magnetic dipoles. A comparison of this result with what was found previously using a representation of the phase dependence Be(Φ) employing a dipole+quadrupole+octupole expansion for the structure shows that this scheme leads only to a formal description of the phase dependence, while the terms in the expansion lack physical significance.

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References

  1. J. D. Landstreet, Astrophys. J. 352, L5 (1990).

    Article  ADS  Google Scholar 

  2. E. Gerth, Yu. V. Glagolevskij, and G. Scholz, in: Stellar Magnetic Fields (1977), Moscow, p. 67.

  3. E. Gerth and Yu. V. Glagolevskij, Bull. Spec. Astrophys. Obs. 56, 25 (2003).

    ADS  Google Scholar 

  4. E. Parker, Cosmic Magnetic Fields [Russian translation], Vol. 1, Mir, (1982).

  5. J. D. Bailey, et al., Mon. Not. Roy. Astron. Soc. 423, 328 (2012).

    Article  ADS  Google Scholar 

  6. Donati,et al., Mon. Not. Roy. Astron. Soc. 291, 658 (1997).

  7. J. D. Landstreet and G. Mathys, Astron. Astrophys. 359, 213 (2000).

    ADS  Google Scholar 

  8. Yu. V. Glagolevskij, Astrophys. Bull. 69 (3), 247 (2014).

    Article  Google Scholar 

  9. O. Kochukhov, et al., Astron. Astrophys. 605, A13 (2017).

    Article  Google Scholar 

  10. Yu. V. Glagolevskij, Astrophys. Bull. 73 (2), 115 (2018).

    Article  Google Scholar 

  11. Yu. V. Glagolevskij, Astrophys. Bull. 75 (4), 440 (2020).

    Article  ADS  Google Scholar 

  12. Yu. V. Glagolevskij, Astrophys. Bull. 66 (2), 144 (2011).

    Article  ADS  Google Scholar 

  13. F. Snik, et al., Astronomical Society of the Pacific Conference Series 437, 237 (2011).

    ADS  Google Scholar 

  14. N. Piskunov, et al., The Messenger 143, 7 (2011).

    ADS  Google Scholar 

  15. O. Kochukhov, et al., Astron. Astrophys. 565, A83 (2014).

    Article  Google Scholar 

  16. Yu. V. Glagolevskij, Astrophys. Bull. 74 (1), 66 (2019).

    Article  ADS  Google Scholar 

  17. Yu. V. Glagolevskij and V. D. Bychkov, Astrophys. Bull. 76 (2), 125 (2023).

    Google Scholar 

  18. Yu. V. Glagolevskij, Astrophisics 59 (3), 321 (2016).

    Article  ADS  Google Scholar 

  19. Yu. V. Glagolevskij, Astrophys. Bull. 71 (1), 43 (2016).

    Article  ADS  Google Scholar 

  20. Yu. V. Glagolevskij, Astrophys. Bull. 79(1), 1 (2024).

    Google Scholar 

  21. G. Mathys and T. Lanz, Astron. Astrophys. 256, 169 (1992).

    ADS  Google Scholar 

  22. G. Mathys, et al., Astron. Astrophys. Suppl. Ser. 123, 353 (1997).

    Article  ADS  Google Scholar 

Download references

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Authors and Affiliations

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

    Yu. V. Glagolevskij

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  1. Yu. V. Glagolevskij
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Correspondence to Yu. V. Glagolevskij.

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Translated from Astrofizika, Vol. 66, No. 4, pp. 539-553 (November 2023).

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Glagolevskij, Y.V. Structure of the Magnetic Field of the Star HD133880 (Si). Astrophysics 66, 503–515 (2023). https://doi.org/10.1007/s10511-024-09806-5

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  • DOI: https://doi.org/10.1007/s10511-024-09806-5

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