Image Details

Choose export citation format:

Atomic Diffusion and Mixing in Old Stars. I. Very Large Telescope FLAMES‐UVES Observations of Stars in NGC 6397

  • Authors: A. J. Korn, F. Grundahl, O. Richard, L. Mashonkina, P. S. Barklem, R. Collet, B. Gustafsson, and N. Piskunov

Korn et al. 2007 The Astrophysical Journal 671 402.

  • Provider: AAS Journals

Caption: Fig. 8.

Observed trends of lithium. Crosses indicate individual stellar abundances, while filled circles show group averages. Solid lines represent the atomic diffusion model predictions (see Fig. 6), which have an original abundance as given by the dashed line [﹩\mathrm{log}\,\varepsilon ( \mathrm{Li}\,) =2.54\pm 0.1﹩]. The dark shaded area shows the predicted primordial lithium abundance ["CMB+BBN:" ﹩\mathrm{log}\,\varepsilon ( \mathrm{Li}\,) =2.64\pm 0.03﹩; Spergel et al. 2007].
Other Images in This Article

Show More

Copyright and Terms & Conditions