  We present a detailed and uniform study of C, S, Zn and Cu abundances in a
large set of planet host stars, as well as in a homogeneous comparison sample
of solar-type dwarfs with no known planetary-mass companions. Carbon abundances
were derived by {EW} measurement of two C I optical lines, while spectral
syntheses were performed for S, Zn and Cu. We investigated possible differences
in the behaviours of the volatiles C, S and Zn and in the refractory Cu in
targets with and without known planets in order to check possible anomalies due
to the presence of planets. We found that the abundance distributions in stars
with exoplanets are the high [Fe/H] extensions of the trends traced by the
comparison sample. All volatile elements we studied show [X/Fe] trends
decreasing with [Fe/H] in the metallicity range -0.8<[Fe/H]<0.5, with
significantly negative slopes of -0.39+-0.04 and -0.35+-0.04 for C and S,
respectively. A comparison of our abundances with those available in the
literature shows good agreement in most cases.
