Lithium Abundance of Metal-poor Stars

High-resolution, high signal-to-noise ratio spectra have been obtained for 32 metal-poor stars. The equivalent widths of Li λ6708A were measured and the lithium abundances were derived. The average lithium abundance of 21 stars on the lithium plateau is 2.33±0.02 dex. The Lithium plateau exhibits a marginal trend along metallicity, dA(Li)/d[Fe/H] = 0.12±0.06, and no clear trend with the effective temperature. The trend indicates that the abundance of lithium plateau may not be primordial and that a part of the lithium was produced in Galactic Chemical Evolution (GCE).

作 者： Hua-Wei Zhang Gang Zhao   作者單位： Hua-Wei Zhang(National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012;Department of Astronomy, School of Physics, Peking University, Beijing 100871;Chinese Academy of Sciences-Peking University Joint Beijing Astrophysical Center, Beijing 100871)

Gang Zhao(National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012) 

刊 名： 天體物理學(xué)報(bào)(英文版)  ISTIC SCI 英文刊名： CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS  年，卷(期)： 2003 3(5)  分類號(hào)： P14  關(guān)鍵詞： stars: abundances - stars: Population Ⅱ - Galaxy: evolution  

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