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Cu and Zn in the early Galaxy

G. Bihain·G. Israelian·R. Rebolo·P. Bonifacio·P. Molaro
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Abstract

We present Cu and Zn abundances for 38 FGK stars, mostly dwarfs, spanning a metallicity range between solar and [Fe/H] =-3. The abundances were obtained using Kurucz's local thermal equilibrium (LTE) model atmospheres and the near-UV lines of CuI 3273.95 A and ZnI 3302.58 A observed at high spectral resolution. The trend of [Cu/Fe] versus [Fe/H] is almost solar for [Fe/H] > -1 and then decreases to a plateau <[Cu/Fe]> =-0.98 at [Fe/H] <-2.5, whereas the [Zn/Fe] trend is essentially solar for [Fe/H] >-2 and then slightly increases at lower metallicities to an average value of <[Zn/Fe]> =+ 0.18. We compare our results with previous work on these elements, and briefly discuss them in terms of nucleosynthesis processes. Predictions of halo chemical evolution fairly reproduce the trends, especially the [Cu/Fe] plateau at very low metallicities, but to a lower extent the greater [Zn/Fe] ratios at low metallicities, indicating eventually missing yields.

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G. Bihain, G. Israelian, R. Rebolo, P. Bonifacio, P. Molaro. 2004-05-04. Cu and Zn in the early Galaxy. https://doi.org/10.1051/0004-6361%3A20035913

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