  We present new measurements of chemical abundances in H II regions in spiral
galaxies of the Virgo cluster and a comparison of Virgo galaxies and field
spirals. With these new data there now exist nine Virgo spirals with abundance
measurements for at least four H II regions. Our sample of Virgo galaxies
ranges from H I deficient objects near the core of the cluster to galaxies with
normal H I properties, far from the cluster core. We investigate the
relationship between H I disk characteristics and chemical abundances to
determine whether dynamical process that remove gas from the disk, such as ram
pressure stripping by the intracluster medium, also affect the chemical
abundances.
