Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-27T10:34:10.477Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Bardeen, J.M., & Petterson, J.A., 1975, ApJ 195, L65 CrossRefGoogle Scholar
Marziani, P., Sulentic, J.W., Dultzin-Hacyan, D., Calvani, M., & Moles, M., 1996, ApJS 104, 37 (M96)CrossRefGoogle Scholar
Thorne, K.S., 1974, ApJ 191, 507 CrossRefGoogle Scholar