CHEMICAL COMPOSITION OF GALACTIC DISK STARS

Автор(и)

  • T. V. Mishenina Astronomical Observatory, Odessa National University T.G.Shevchenko Park, Odessa 65014 Ukraine, Ukraine
  • N. Yu. Basak Astronomical Observatory, Odessa National University T.G.Shevchenko Park, Odessa 65014 Ukraine, Ukraine
  • T. I. Gorbaneva Astronomical Observatory, Odessa National University T.G.Shevchenko Park, Odessa 65014 Ukraine, Ukraine
  • C. Soubiran Observatoire Aquitain des Sciences de l'Univers CNRS UMR 5804, BP 89, 33270 Floirac, France, France
  • V. V. Kovtyukh Astronomical Observatory, Odessa National University T.G.Shevchenko Park, Odessa 65014 Ukraine, Ukraine

DOI:

https://doi.org/10.18524/1810-4215.2007.20.87160

Ключові слова:

Stars, fundamental parameters, stars, abundances

Анотація

Abundances of Na, Al, Ca, in the stars of galactic disks are obtained. The separation of thin and stars on cinematic criterion was made early. The behavior of chemical element abundances with metallicity for studied stars was presented.

Посилання

Galazutdinov G.A.: 1992, Preprint SAO RAS, 92.

Katz D., Soubiran C., Cayrel R. et al.: 1998, A&A, 338, 151.

Kovtyukh V.V., Andrievsky S.M.: 1999, A&A, 351, 597.

Kovtyukh V.V., Soubiran C. et. al: 2003, A&A, 411, 559.

Kurucz R.L.: 1993, CD ROM, 13.

Mishenina T.V., Soubiran C., Kovtyukh V.V.: 2004, A&A, 418, 551.

Tsymbal V.V.: 1996, ASP Conf. Ser., 108, 198.

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Опубліковано

2007-12-22

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