Virgo cluster galaxies observed in radio continuum emission. Blue: VLA 6 cm total power; green: VLA 6 cm polarized emission, red: ROSAT intracluster medium X-ray emission (from Böhringer et al. 1994). The galaxies are located at the proper position in the cluster but each radio continuum image is magnified by a factor 10 to show the details of the radio continuum distribution. Radio continuum point sources from the VLA images were not removed. The VLA radio continuum data are from this paper, Vollmer et al. (2010), Vollmer et al. (2004a; NGC 4522), and Chyży et al. (2007; NGC 4254).