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Chemical compositions of photometric solar-analog stars and F-G stars of different ages

Published online by Cambridge University Press:  23 December 2005

I. Bikmaev ,
A. Galeev ,
N. Sakhibullin  and
F. Musaev
I. Bikmaev
Affiliation:
Kazan State University and Academy of Sciences of Tatarstan, Kazan, 420111, Russia email: Ilfan.Bikmaev@ksu.ru
A. Galeev
Affiliation:
Kazan State University and Academy of Sciences of Tatarstan, Kazan, 420111, Russia email: Ilfan.Bikmaev@ksu.ru
N. Sakhibullin
Affiliation:
Kazan State University and Academy of Sciences of Tatarstan, Kazan, 420111, Russia email: Ilfan.Bikmaev@ksu.ru
F. Musaev
Affiliation:
Special Astrophysical Observatory of Russian Academy of Sciences, Karachai-Cherkessian Republic, 369167, Russia email: faig@sao.ru
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Abstract

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We present the main results of our study of photometric solar-analog stars.

Keywords

Stars: abundancestechniques: spectroscopic