  We present the first results of the estimation of gravity and effective
temperature for some poorly studied chemically peculiar stars that were
recently observed with the spectropolarimeter ESPaDOnS at CFHT. We have
analyzed the spectra of HD71030, HD95608 and HD116235 to determine their radial
velocity, Vsin(i) and the average abundance of several chemical species. We
have also analyzed our results to verify for possible vertical abundance
stratification of iron and chromium in these stars.
