Using CASLEO echelle spectrograms, elemental abundances are derived fo
r the sharp-lined nonmagnetic CP stars HR 4487, 14 Hya, and 3 Cen A. T
he first two stars are members of the Mercury-Manganese subgroup and h
ave abundances which are similar to other such peculiar stars. The thi
rd is a hotter related star. The detection of Mn II lines in its spect
rum adds to this relationship(1).