We present the results of our recent search for pulsational line profile variations in high time resolution UVES spectra of the most evolved Ap star known , the \delta Scuti star HD 21190 , and of the Ap Sr star HD 218994 .
We found that HD 218994 is an roAp star with a pulsation period of 5.1 min , which makes it the 36 ^ { th } star known to be a roAp star .
No rapid pulsations have been found in the spectra of the \delta Scuti star HD 21190 .
However , we detect moving peaks in the cores of spectral lines , which indicate the presence of non-radial pulsations in this star .