On the Abundances of Heavy Elements in the Atmosphere of GAM Tauri

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The comparison of the spectral atlases of Gamma Tauri with synthetic spectra permit us to identify absorption lines of iron and heavy elements. We determined the abundances of iron and 20 elements with Z>=29 in the atmosphere of this K-giant of Hyades cluster, in order to verify the possible enhancements of chemical abundances of stars in young clusters. Spectrum synthesis and model atmosphere methods were used. Molecular lines, hyperfine and isotopic structure for some elements were taken in account. All values of abundances of investigated elements in the atmosphere of Gamma Tauri are close to solar values.

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