SUBDWARFS: ABUNDANCE OF LIGHT ELEMENTS

Автор(и)

  • T. V. Mishenina Astronomical Observatory, Odessa State University, Ukraine
  • V. G. Klochkova Special Astrophysical Observatory, Russian Academy of Sciences, Russian Federation
  • V. E. Panchuk Special Astrophysical Observatory, Russian Academy of Sciences, Russian Federation

DOI:

https://doi.org/10.18524/1810-4215.1996.9.109489

Ключові слова:

stars, abundances, atmospheres, evolution

Анотація

CNO abundances in the atmospheres of seven metal-deficient stars were derived by model atmosphere method on the basis of high dispersion Echelle spectra obtained using the 6-m telescope of the Special Observatory of the Russian Academy of Sciences. The O abundances are derived from lines of lR-triplet Ol 7773 Å. The C2(0,1) bandhead of the Svaan A3IIg – X3llg system, at 5635.5 Å is used to derive the C abundances. To derive the nitrogen abundances, the CN red system A2ll-X2Σ was used. the CN(5,1) 6332.18 Å and 6478.48 Å were considered. The obtained [O/Fe] values confirm the trend of [O/Fe] vs [Fe/H]. For stars of our sample with [Fe/H] > -1.00 we found that nitrogen is overabundant relative to iron; carbon - underabundant.

Посилання

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2017-09-04

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