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Isotopic Lithium Abundances in Nine Halo Stars

  • Authors: Verne V. Smith, David L. Lambert, and Poul E. Nissen

Smith, Lambert, & Nissen 1998 The Astrophysical Journal 506 405.

  • Provider: AAS Journals

Caption: Fig. 3.

Fitting procedure for HD 74000. The top left panel shows the observed Ca I 6162 Å line (open circles) and synthetic spectra for three values of Γ. The top right panel shows the reduced χ2 residuals as a function of the macroturbulence. The bottom left panel is the observed Li I line (open circles) and synthetic spectra for three values of f(6Li). The bottom right panels illustrates the reduced χ2 residuals vs. 6Li fraction for three values of the macroturbulence.

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