Image Details
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.
© 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.