Using population synthesis methods we determined the relative stellar
components around Seyfert nuclei in their host galaxies and the nonthe
rmal flux contribution from the nuclei. Knowing the stellar components
from the spatially resolved spectra of our objects we can calculate t
he number of OB-stars and from that the star formation rate. We found
that the contribution of OB-stars is correlated with the strength of t
he nonthermal flux at the nucleus.