Abstract
Curve-of-growth analyses with respect to ζ Cap for the coolest BaII star HD 121447 and the CS star R CMi have been made, and physical parameters and relative abundances of the elements have been determined. In HD 121447 s-process elements are overabundant by factors of about 10-30, while in R CMi they are overabundant by factors of about 30-100.
