Abstract:
We discuss results from very long baseline interferometry (VLBI)
observations of two Seyfert galaxies with double peaked emission lines in
their SDSS optical spectra. Such AGN are potential candidates for the
presence of binary black holes, which can be resolved on parsec-scales
with VLBI. Our observations do not detect twin radio cores but rather nuclear outflows in these Seyferts. These outflows could be interacting with
the emission line clouds producing the double peaks in the emission lines