New procedure of the fine analysis of spectra of F-G-K stars
1 Main Astronomical Observatory of the National Academy of Sciences
2 University of Hertfordshire
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Some problems of the determination of the microturbulent velocities and abundances in atmospheres of the F-G-K stars and determination of their effective temperatures and rotational velocities in the framework of self-consistent approach are discussed. Firstly, we use independent determinations of iron abundances. using the fits to the observed profiles of Fe I and Fe II absorption lines. Secondly, abundances of other elements are determined for the found input parameters.
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