  We present a differential abundance analysis of Hyades F-K dwarfs in search
for evidence of stellar enrichment from accreted hydrogen deficient disk
material. Metallicites and relative abundance ratios of several species have
been determined. We derive a cluster mean [Fe/H] = 0.13+-0.01. Two stars show
abundances ~0.2 dex larger than the cluster mean. Additionally, one star, which
was added by a recent study as a cluster member, shows significantly lower
abundances than the cluster mean. These three stars have questionable
membership characteristics. The remaining stars in the survey have an rms of
0.04 dex in the differential [Fe/H] values. The Hyades cluster members have
apparently not been significantly chemically enriched. The abundance ratios of
Si, Ti, Na, Mg, Ca and Zn with respect to Fe are in their solar proportions.
