Can the Formation of X-ray Obscuring Tori and Jets in Active Galaxies be Determined by One Parameter?

A torus of reduced differential rotation can form in the inner $\text{siml}10$pc core of active galactic nuclei incurring a density enhancement that can account for obscuration of X-rays in Seyferts when the initial inner core to black hole mass ratio $\text{gsim}50$. The same density enhancement and reduction in differential rotation can also lead to dynamo growth of poloidal fields which attain a magnitude $\sim {10}^4$G when accreted onto the central engine. As radio jet models often employ poloidal fields as agents in extracting power for the jet luminosity, we suggest that jetted AGN might require this poloidal field production. Although the poloidal field would be originally produced in the obscuring torus, jetted objects are less likely to have obscuring tori: The poloidal field would only aid in powering jet emission after it accretes with the torus matter to the central engine. Thus, only during the relatively short torus accretion time scale could there be both a jet and and torus.