Chemical abundance patterns – fingerprints of nucleosynthesis in the first stars
Department of Astronomy and Space Physics, Uppsala Astronomical Observatory, Box 515, 751 20 Uppsala, Sweden
Corresponding author: T. Karlsson, Torgny.Karlsson@astro.uu.se
Figures 17 and 18 on page 478 were misprinted. The metallicity of the stars, measured by [Fe/H], was wrongly indicated and one star was missing. The corrected figures are shown below. No conclusions are altered.
© ESO, 2002