CHEMICAL ABUNDANCES IN BINARIES WITH TWIN COMPONENTS

Автор(и)

  • Yu. Lyubchik Main Astronomical Observatory of NASU, Kiev 03680 Ukraine, Ukraine
  • E. Martin Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu HI, 96822, USA, United States
  • G. Basri Astronomy Department, University of California, Berkeley, CA 94720, USA, United States
  • Ya. Pavlenko Main Astronomical Observatory of NASU, Kiev 03680 Ukraine, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2001.14.99465

Ключові слова:

Stars, binary stars, chemical abundances.

Анотація

Procedure and some preliminary results of abundances determination in binaries with twin components from solar neighborhood are discussed. Numerical analysis were carried out by fits of synthetical spectra and COG to high resolution (R=50000) observed data. To fit the observations we used model atmospheres of Kurucz with different metallicities and (modified) VALD line list.

Посилання

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2017-04-20

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