CHEMICAL COMPOSITION OF COOL GIANT STARS

Автор(и)

  • N. S. Komarov Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 270014 Ukraine., Ukraine
  • N. J. Basak Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 270014 Ukraine., Ukraine
  • T. I. Gorbaneva Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 270014 Ukraine., Ukraine
  • L. E. Kantsen Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 270014 Ukraine., Ukraine

DOI:

https://doi.org/10.18524/1810-4215.1994.7.105750

Ключові слова:

Stars, abundances, giant

Анотація

Based upon the catalogue of equivalent widths of absorption lines in spectra of cool giant - stars created at the Astrospectroscopy Department of the Astronomical Observatory in Odessa the abundances in their atmospheres is determined. This determination was made by using the method of model atmospheres. Fundamental characteristics of stars are determined by an independent method by using photometric observations.

Посилання

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Korotina L.V., Dragunova A.V., Komarov N.S.: 1988, Preprint UkrNIINTI, 2037.

Korotina L.V., Dragunova A.V., Komarov N.S.: 1989, Astrofizika, 31, 539.

Korotina L.V., Komarov N.S.: 1992, Astron.Zhurn., 69, 1188.

Kurucz R.L., Peytremann E.: 1975, Spec.Rept.SAO, 362, 401.

Motrich V.D,: 1990, Preprint UkrNIINTI,1926.

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2017-07-01

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