NON-STATIONARY HE-WEAK STAR HD182255?

Автор(и)

  • Yu. V. Glagolevskij Special Astrophysical Observatory of Russian Academy of Sciences, Російська Федерація
  • A. V. Shavrina Main Astronomical Observatory of National Academy of Sciences of Ukraine, Україна
  • G. A. Chuntonov Special Astrophysical Observatory of Russian Academy of Sciences, Російська Федерація

DOI:

https://doi.org/10.18524/1810-4215.2010.23.84145

Ключові слова:

Stars, He-weak, magnetic field, stars, individual, HD182255, 3 Vul

Анотація

It is known that the chemical elements distribution on the surface of chemically peculiar (CP) stars are associated with the distribution of the magnetic field. It is interest to study CP stars of various types and temperatures for the distribution of chemical elements on the surface. To this aim our research program includes HgMn star HD 182255 with no magnetic field, but with spectral and photometric variability, which is unusual in terms of the aforementioned. We suspect that the non-uniform distribution of helium and silicon on the surface of the star is due to the influence of the weak magnetic field.

 

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Опубліковано

2010-11-23

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