The Point of Origin of the Radio Radiation from the Unresolved Cores of Radio-Loud Quasars

Abstract

Locating the exact point of origin of the core radiation in active galactic nuclei (AGN) would represent important progress in our understanding of physical processes in the central engine of these objects. However, due to our inability to resolve the region containing both the central compact object and the jet base, this has so far been difficult. Here, using an analysis in which the lack of resolution does not play a significant role, we demonstrate that it may be impossible even in most radio loud sources for more than a small percentage of the core radiation at radio wavelengths to come from the jet base. We find for 3C279 that $\sim 85$ percent of the core flux at 15 GHz must come from a separate, reasonably stable, region that is not part of the jet base, and that then likely radiates at least quasi-isotropically and is centered on the black hole. The long-term stability of this component also suggests that it may originate in a region that extends over many Schwarzschild radii.

7 pages with 3 figures, accepted for publication in Astrophysics and Space Science

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Cited by in corpus (5)

• X-ray Emission from Optically Selected Radio-Intermediate and Radio-Loud Quasars
• Intra-night optical variability of core dominated radio quasars: the role of optical polarization
• Doppler Boosting May Have Played No Significant Role in the Finding Surveys of Radio-Loud Quasars
• Evidence that the Bursting Component of the X-ray Radiation From 3C 111 Originates in the PC-Scale Jet
• On The Depolarization Asymmetry Seen in Giant Radio Lobes