LITHIUM BLEND FITTING FOR roAp STAR HD101065 (PRZYBYLSKI'S STAR)

Автор(и)

  • A. V. Shavrina Main Astronomical Observatory of NAS of Ukraine, Golosiivo, 03650, Kyiv, Ukraine, Ukraine
  • V. Khalack Main Astronomical Observatory of NAS of Ukraine, Golosiivo, 03650, Kyiv, Ukraine, Ukraine
  • N. S. Polosukhina Crimean Astrophysical Observatory, Nauchnyj, Crimea, Ukraine, Ukraine
  • J. Zverko Astronomical Institute of the Slovak Academy of Sciences, 05960 Tatranska Lomnica, the Slovak Republic, Slovakia
  • J. Zhiznovsky Astronomical Institute of the Slovak Academy of Sciences, 05960 Tatranska Lomnica, the Slovak Republic, Slovakia
  • V. F. Gopka Astronomical observatory, Odessa National University, 65014, park Shevchenko, Odessa, Ukraine, Ukraine
  • P. North Inst. d'Astronomie, Univ. Lausanne, CH-1290 Chavannes-des-Bois, Switzerland, Switzerland
  • V. V. Tsymbal Tavrian National University, Simpheropol, Ukraine, Ukraine
  • A. V. Yushchenko Astronomical observatory, Odessa National University, 65014, park Shevchenko, Odessa, Ukraine, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2001.14.99495

Ключові слова:

Stars, chemically peculiar, individual, HD101065 stars, HD101065.

Анотація

We have considered the possibility for modeling of remarkable spectral feature 6708 Å for HD101065 (Przybylski's star) in two ways - as a blend of Li and REE lines and as blend of REE lines only. We show by model calculations that Li lines absorb significantly in the range 6707.72-6708.02 ÅÅ and resulting Li abundance 3.3 dex (in the scale lg N(H)=12.0) is near to the primordial value.

Посилання

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2017-04-20

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