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On the Difference Between Radio Quiet and Radio Loud AGN
Published online by Cambridge University Press: 12 April 2016
Abstract
A systematic difference in alignment between the central black hole spin and the angular momentum of the accreting gas may help to explain several differences found in the optical and UV HST spectra of radio loud and radio quiet AGN.
- Type
- Part 15. Poster Papers
- Information
- International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 761 - 762
- Copyright
- Copyright © Astronomical Society of the Pacific 1997
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