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LITHIUM ABUNDANCES OF EXTREMELY METAL-POOR TURNOFF STARS*

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Wako Aoki1,2, Paul S. Barklem3, Timothy C. Beers4, Norbert Christlieb5, Susumu Inoue1,9, Ana E. García Pérez6, John E. Norris7 and Daniela Carollo7,8

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We have determined Li abundances for eleven metal-poor turnoff stars, among which eight have [Fe/H] <–3, based on LTE analyses of high-resolution spectra obtained with the High Dispersion Spectrograph on the Subaru Telescope. The Li abundances for four of these eight stars are determined for the first time by this study. Effective temperatures are determined by a profile analysis of Hα and Hβ. While seven stars have Li abundances as high as the Spite Plateau value, the remaining four objects with [Fe/H] <–3 have A(Li) =log (Li/H)+ 12 lsim 2.0, confirming the existence of extremely metal-poor (EMP) turnoff stars having low Li abundances, as reported by previous work. The average of the Li abundances for stars with [Fe/H]<–3 is lower by 0.2 dex than that of the stars with higher metallicity. No clear constraint on the metallicity dependence or scatter of the Li abundances is derived from our measurements for the stars with [Fe/H]<–3. Correlations of the Li abundance with effective temperatures, with abundances of Na, Mg, and Sr, and with the kinematical properties are investigated, but no clear correlation is seen in the EMP star sample.


Footnote
*  Based on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan.
Keywords

nuclear reactions, nucleosynthesis, abundances; stars: abundances; stars: Population II


Dates

Issue 2 (2009 June 20)

Received 2008 November 26, accepted for publication 2009 April 13

Published 2009 June 4



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