On the Difference Between Radio Quiet and Radio Loud AGN
arXiv:astro-ph/9609032
Abstract
A systematic difference in alignment between the central black hole spin and the angular momentum of the accreting gas may help explain several differences found in the optical and UV HST spectra of radio loud and radio quiet AGN.
2 pages, to appear in Accretion Phenomena and Related Outflows, Proceedings of the IAU Symp. # 163