Abstract:
We present our results from FUSE observations of Seyfert galaxies of type 2 (Sy 2). We attempt to contrast the properties of the emission lines and absorbing outflows in Sy 1s and 2s in the framework of Unification. We find that the O VI emission in Sy 2s is narrow as predicted. We also find evidence for absorption, and blue-ward asymmetry of the O VI line profile.
