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On the Difference Between Radio Quiet and Radio Loud AGN

Published online by Cambridge University Press:  12 April 2016

P. Marziani ,
M. Calvani  and
J. W. Sulentic
P. Marziani
Affiliation:
Osservatorio Astronomico di Padova, Italia
M. Calvani
Affiliation:
Osservatorio Astronomico di Padova, Italia
J. W. Sulentic
Affiliation:
University of Alabama, Tuscaloosa, USA

Abstract

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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

References

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Marziani, P., Sulentic, J.W., Dultzin-Hacyan, D., Calvani, M., & Moles, M., 1996, ApJS 104, 37 (M96)CrossRefGoogle Scholar
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