On the Difference Between Radio Quiet and Radio Loud AGN

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dc.creatorMarziani, P.
dc.creatorCalvani, M.
dc.creatorSulentic, J. W.
dc.date1996-09-04
dc.date.accessioned2026-07-07T02:21:51Z
dc.date.available2026-07-07T02:21:51Z
dc.descriptionA 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.
dc.description2 pages, to appear in Accretion Phenomena and Related Outflows, Proceedings of the IAU Symp. # 163
dc.identifierhttps://arxiv.org/abs/astro-ph/9609032
dc.identifierhttp://arxiv.org/abs/astro-ph/9609032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10661
dc.subjectAstrophysics
dc.titleOn the Difference Between Radio Quiet and Radio Loud AGN
dc.typetext

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