  As a part of an on-going program to explore the signature of p-modes in
solar-like stars by means of high-resolution absorption lines pectroscopy, we
have studied four stars (alfaCMi, etaCas A, zetaHer A and betaVir). We present
here new results from two-site observations of Procyon A acquired over twelve
nights in 1999. Oscillation frequencies for l=1 and l=0 (or 2) p-modes are
detected in the power spectra of these Doppler shift measurements. A frequency
analysis points out the dificulties of the classical asymptotic theory in
representing the p-mode spectrum of Procyon A.
