Effective temperatures and lithium abundances of halo turnoff stars
Effective temperatures of 30 turnoff stars with -3.2 {[Fe/H]{ have been derived from the profiles of Balmer lines in high S/N, VLT/UVES spectra. While the systematic error of Teff may be of the order of 100K, the differential values of Teff are determined with a one-sigma precision of ˜25K. These precise Teff values are used in a study of the slope
Nissen, P. E. et al.
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2005