  The Optical Monitor telescope (Mason et al. 2001) on XMM-Newton provides an
exciting multi-wavelength dimension to observations of Active Galactic Nuclei.
Here we present ultraviolet images, taken with the OM UVW2 filter (140-270 nm),
of various Seyfert galaxies, some of which have never been observed in this
waveband before. The images show UV emission from both the active nucleus and
the host galaxy. The distribution of UV emission in the galaxy shows where star
formation is occurring, thus giving us clues as to the evolution of the host
galaxy and perhaps its relationship to the Seyfert Nucleus.
