Evolution from the nuclides to the chemical elements

Автор(и)

  • N. S. Komarov Astronomical Observatory, Odessa National University, Україна

DOI:

https://doi.org/10.18524/1810-4215.2002.15.95043

Ключові слова:

stars, fundamental characteristics, abundances, nucleosynthesis, evolution

Анотація

The chemical evolution of Universe and it's objects (from grains to black holes) were of main goal of recent reviews and investigations. The evolution of chemical elements and their isotopes (early nuclides) discussed as indicator of evolution of Universe from Big Bang to now. The problem of determination of contents of chemical elements and their isotopes in atmospheres of cool giants to use method of the models of atmospheres and the synthetic spectra is discussed briefly. The determination of fundamental characteristics of cool stars (the effective temperature Teff , surface gravity lgg, metallicity [Fe/H]) are discussed too. The evolution of all nuclides heaver 4He (with the exception, possibly, of most lightest nuclides - 6Li, 7Li, 9Be, 10B, 11B) are caused of these stars.

Посилання

Anders Е.. Grevesse N.: 1989, Geoch. Cosmoch. Acta, 53, 197.

Bell R.A., Eriksson R., Gustafsson В., Nordlund А.: 1978, Astron. Astrophys. Suppl, 34, 229.

Cameron A.J . Contents of chemical elements and nuclides in solar system. 1986, The nuclear Astrophysics /ed. D.D. Clayton, D.N. Schramun, Gehren T.: 1988, Rev. in Modem Astrommy, 1, 52.

Gopka V.F., Komarov N.S., Mishenina T.V, Yushchenko A.V.; 1990a, Astron. Zurnal, 67, 1204.

Gopka V.F., Komarov N.S.: 1990b, Astronom. Zurnal., 67, 1211

Gratton R.G., Sneden C.: 1987, Astron. Astrophys.,

, 179.

Grevesse N ., Sauval A.J., Standard Solar Composition. Space Science Rewiews, 1998, 85, 161-174.

Kjargaard P., Gustafsson E., Walker G.A.K., Hulftgwist L.: 1987, Astrcm. Astrophy3.. 178, 145.

Komarov N .S., Mishenina T.V.: 1985a, Kinematika i fizika nebesnych tel, 1, 77.

Komarov N.S., Mishenina T.V., Motrich V.D.: 1985b), Astron. Zurnal, 62, 740.

Komarov N.S., Basak N.Yu.: 1992. Astron. Astrophys. Trans., 3, 179.

Kumarov N.S., Basak N.Ju., Gorbaneva T.V., Kantzen L.E.: 1994, Odessa Аstrоп. Рubl.‚ 7, 143.

Komarov N.S.. Korotina L.V., Shevchuk T.V.: 1996, Kinematika i fisika nebesnych tel, 26, 3

Komarov N.S.: 1999, The cool stars-giant, Astroprint, Odessa, 213 p. (Rus.)

Komarov N.S., Zgonyajko N.S., Vasil'eva S.V.: 2001, Kinematika і fizika nebesnych tel, 17, 471.

Korotina L.V., Dragunova А.V., Komarov N.S.: 1989. Astrophysika, 21. 9.

Кorotina L.V., Кomarov N.S.: 1992, Аstron. Zurnal, 69, 1188.

Kovtyukh V.V., Komarov N.S., Andrievsky S.М., Dulapchi I.Р.: 2000, Odessa Аstron. Publ., 12.

Kurucz R.L.: 1993, CD-ROM N18, Smithsonian Astrophys. Obs. Cambridge, MA

Lyubimkov L.S. The chemical content: the methods and results of analisis. 1995, Astroprint, Odessa, 324 p. (Rus.)

Mishenina T.V., Panchuk V.E., Komarov N.S. 1986, Izvestia SAO. 28. 1.

Ridgway S.T., Joyce R.R., White N.M., Wing H.F.: 1980, Astrophys. J., 235. 126.

Rykaljuk: 1998, The elected problems of astronomy and astrophysics, L’vov. 58.

Sweigart A.V., Greggio L., Renzini A.: 1989. Astrophys. J. Suppl., 69, 911 p.

Trimble V.: 1975. Reviews of Modern Physics, 47, N4, 976 p.

Trimble V.: 1991, Astrophys. Rev., 3, 1.

Tsymbal V.V.: 1994, Odessa Astron. Publ., 7, 146.

Tsymbal V.V.: 1995, ASP Conference Ser, 108, 198.

Zinner E., Amari S.: 1999, Asymptotic Giant Branch Stars, IAU. Symposium 191, 59-68.

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2017-03-07

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